<rss version="2.0">
<channel>
<title>sci.astro.research :: Forum in astronomy/astrophysics research. (Moderated)</title>
<link>http://www.nnseek.com/e/sci.astro.research/</link>
<description>Posts for sci.astro.research</description>
<lastBuildDate>Mon, 22 Sep 2008 03:05:32 PDT</lastBuildDate>
  <image>
    <title>http://www.nnseek.com/</title>
    <link>http://www.nnseek.com/</link>
    <url>http://www.nnseek.com/img/64.png</url>
    <width>64</width>
    <height>64</height>
    <description>NNSeek</description>
  </image>
<item>
	<title><![CDATA[&quot;Stars Lie With Enormous Disk of Dark Matter&quot;]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/stars_lie_with_enormous_disk_of_dark_matter_116937465t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/stars_lie_with_enormous_disk_of_dark_matter_116937465t.html</link>
	<description><![CDATA[Participants here may enjoy reading this rather<br>fluff level ScienceNOW article from Science<br>Magazine, suggesting that there has now been found a<br>more detailed structure of the sphere of dark matter<br>within which a galaxy is embedded:<br><br><a href="http://sciencenow.sciencemag.org/cgi/content/full/2008/916/2?etoc" rel="nofollow" class="url" target="_blank">http://sciencenow.sciencemag.org/cgi/content/full/2008/916/2?etoc</a><br><br>FYI<br><br>xanthian.<br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/stars_lie_with_enormous_disk_of_dark_matter_116937465t.html">no comments</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/stars_lie_with_enormous_disk_of_dark_matter_116937465m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Mon, 22 Sep 2008 03:05:32 PDT</pubDate>
</item>
<item>
	<title><![CDATA[[WWW] Illusory velocity]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/www_illusory_velocity_116891129t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/www_illusory_velocity_116891129t.html</link>
	<description><![CDATA[The theory is done and I am finally into the section of the website<br>where I look at observational evidence. Two new pages<br><br><a href="http://www.teleconnection.info/rqg/GalaxyRotationCurves" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/GalaxyRotationCurves</a><br><br>discusses the evidence for and against CDM and MOND, and compares to the<br>predictions of the teleconnection given in<br><br><a href="http://www.teleconnection.info/rqg/QuantumCoordinates" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/QuantumCoordinates</a><br><br>The teleconnection does not require exotic CDM or a modification to<br>Newtonian gravity, but instead predicts that redshifts from astronomical<br>bodies need to be reinterpreted to take account of a term dependent on<br>cosmological expansion.<br><br>Regards<br><br>-- <br>Charles Francis<br>moderator sci.physics.foundations.<br>charles (dot) e (dot) h (dot) francis (at) <a href="http://googlemail.com" rel="nofollow" class="url" target="_blank">googlemail.com</a> (remove spaces and<br>braces)<br><br><a href="http://www.teleconnection.info/rqg/MainIndex" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/MainIndex</a><br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/www_illusory_velocity_116891129t.html">no comments</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/www_illusory_velocity_116891129m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Sun, 21 Sep 2008 02:44:49 PDT</pubDate>
</item>
<item>
	<title><![CDATA[Pioneer]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/pioneer_116241145t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/pioneer_116241145t.html</link>
	<description><![CDATA[I have added a short discussion of the Pioneer blueshift, and the<br>calculation showing it is predicted by the teleconnection.<br><br>I recently found two papers containing essentially the same calculation<br>(referenced on the webpage)<br><br><a href="http://www.teleconnection.info/rqg/Pioneer" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/Pioneer</a><br><br>Regards<br><br>-- <br>Charles Francis<br>moderator sci.physics.foundations.<br>charles (dot) e (dot) h (dot) francis (at) <a href="http://googlemail.com" rel="nofollow" class="url" target="_blank">googlemail.com</a> (remove spaces and<br>braces)<br><br><a href="http://www.teleconnection.info/rqg/MainIndex" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/MainIndex</a><br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/pioneer_116241145t.html">no comments</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/pioneer_116241145m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Mon, 15 Sep 2008 01:02:09 PDT</pubDate>
</item>
<item>
	<title><![CDATA[Will Sirius Supernova, and if so when?]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/will_sirius_supernova_and_if_so_when_115659769t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/will_sirius_supernova_and_if_so_when_115659769t.html</link>
	<description><![CDATA[Sirius A is a main sequence star, of about 2 solar masses, and its<br>companion Sirius B is a white dwarf of about 1 solar masses. Once Sirius<br>A goes giant, it is possible that matter will be sucked into Sirius B.<br>If Sirius B thereby reaches the Chandrasekhar limit of 1.4 Solar masses,<br>it will supernova.<br><br>Can anyone estimate whether this process will actually take place, and<br>if so when? At nine light years, what would be the effect on Earth?<br><br><br><br>Regards<br><br>-- <br>Charles Francis<br>moderator sci.physics.foundations.<br>charles (dot) e (dot) h (dot) francis (at) <a href="http://googlemail.com" rel="nofollow" class="url" target="_blank">googlemail.com</a> (remove spaces and<br>braces)<br><br><a href="http://www.teleconnection.info/rqg/MainIndex" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/MainIndex</a><br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/will_sirius_supernova_and_if_so_when_115659769t.html"><b>1</b> Comment</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/will_sirius_supernova_and_if_so_when_115659769m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Wed, 10 Sep 2008 05:00:44 PDT</pubDate>
</item>
<item>
	<title><![CDATA[GRB 19 Mar 2008]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/grb_19_mar_2008_115635705t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/grb_19_mar_2008_115635705t.html</link>
	<description><![CDATA[I read about the above Gamma Ray Burst,<br>but days,weeks, months later no published analysis<br>materialized, that I have found.  Are the astronomers<br>still consolidating the data for peer publication?<br>Anyway what's the "fallout" ?<br>I quite interested in a "neutrino shock wave" that<br>occurred like SN1987a, but this burst, at a greater<br>distance, might produce a definite variation of the<br>neutrino speed to light speed.<br>Comments very welcome.<br>Regards<br>Ken S. Tucker<br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/grb_19_mar_2008_115635705t.html">no comments</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/grb_19_mar_2008_115635705m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Wed, 10 Sep 2008 00:50:10 PDT</pubDate>
</item>
<item>
	<title><![CDATA[[WWW] Supernova fits and cosmological parameters]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/www_supernova_fits_and_cosmological_parameters_115363065t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/www_supernova_fits_and_cosmological_parameters_115363065t.html</link>
	<description><![CDATA[I am on the final section of the website, in which I compare the<br>predictions of relational quantum gravity with observation and with<br>those of standard cosmology. I have posted the results of the supernova<br>analysis, with graphs,  and comparison of the properties of the models<br><br><a href="http://www.teleconnection.info/rqg/Supernova" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/Supernova</a><br><br><br><br>Regards<br><br>-- <br>Charles Francis<br>moderator sci.physics.foundations.<br>charles (dot) e (dot) h (dot) francis (at) <a href="http://googlemail.com" rel="nofollow" class="url" target="_blank">googlemail.com</a> (remove spaces and<br>braces)<br><br><a href="http://www.teleconnection.info/rqg/MainIndex" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/MainIndex</a><br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/www_supernova_fits_and_cosmological_parameters_115363065t.html"><b>4</b> Comments</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/www_supernova_fits_and_cosmological_parameters_115363065m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Mon, 08 Sep 2008 12:48:56 PDT</pubDate>
</item>
<item>
	<title><![CDATA[More puzzles for CDM]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/more_puzzles_for_cdm_114639609t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/more_puzzles_for_cdm_114639609t.html</link>
	<description><![CDATA[It seems as though smaller galaxy are more dominated by CDM.<br><br><a href="http://arxiv.org/PS_cache/arxiv/pdf/0808/0808.3772v1.pdf" rel="nofollow" class="url" target="_blank">http://arxiv.org/PS_cache/arxiv/pdf/0808/0808.3772v1.pdf</a><br><br>Regards<br><br>-- <br>Charles Francis<br>moderator sci.physics.foundations.<br>charles (dot) e (dot) h (dot) francis (at) <a href="http://googlemail.com" rel="nofollow" class="url" target="_blank">googlemail.com</a> (remove spaces and<br>braces)<br><br><a href="http://www.teleconnection.info/rqg/MainIndex" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/MainIndex</a><br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/more_puzzles_for_cdm_114639609t.html">no comments</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/more_puzzles_for_cdm_114639609m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Tue, 02 Sep 2008 22:38:46 PDT</pubDate>
</item>
<item>
	<title><![CDATA[supernova data]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/supernova_data_114282233t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/supernova_data_114282233t.html</link>
	<description><![CDATA[There has been a new, and substantially larger compilation including new<br>near SN (which should much improve the dataset) , while I wasn't looking<br><br><a href="http://arxiv.org/abs/0804.4142" rel="nofollow" class="url" target="_blank">http://arxiv.org/abs/0804.4142</a><br><br>They have a website where they intend to keep regular updates, and from<br>which the data can be downloaded.<br><br><a href="http://supernova.lbl.gov/Union" rel="nofollow" class="url" target="_blank">http://supernova.lbl.gov/Union</a>/<br><br><br><br>Regards<br><br>-- <br>Charles Francis<br>moderator sci.physics.foundations.<br>charles (dot) e (dot) h (dot) francis (at) <a href="http://googlemail.com" rel="nofollow" class="url" target="_blank">googlemail.com</a> (remove spaces and<br>braces)<br><br><a href="http://www.teleconnection.info/rqg/MainIndex" rel="nofollow" class="url" target="_blank">http://www.teleconnection.info/rqg/MainIndex</a><br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/supernova_data_114282233t.html"><b>6</b> Comments</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/supernova_data_114282233m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Mon, 01 Sep 2008 02:18:51 PDT</pubDate>
</item>
<item>
	<title><![CDATA[bright blue 1-4 pixel sources on darker 3D fractal web in IR and]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/bright_blue_1_4_pixel_sources_on_darker_3d_fractal_111062009t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/bright_blue_1_4_pixel_sources_on_darker_3d_fractal_111062009t.html</link>
	<description><![CDATA[bright blue 1-4 pixel sources on darker 3D fractal web in IR and<br>visible light HUDF images: Rich Murray 2008.08.05<br><a href="http://rmforall.blogspot.com/2008_07_01_archive.htm" rel="nofollow" class="url" target="_blank">http://rmforall.blogspot.com/2008_07_01_archive.htm</a><br>Thursday, July 31, 2008<br><a href="http://groups.yahoo.com/group/AstroDeep/24" rel="nofollow" class="url" target="_blank">http://groups.yahoo.com/group/AstroDeep/24</a><br><a href="http://groups.yahoo.com/group/rmforall/84" rel="nofollow" class="url" target="_blank">http://groups.yahoo.com/group/rmforall/84</a><br><br><br>Hubble Infrared Ultra Deep Field clearly reveals deep cosmic<br>background fractal 3D mesh of H filaments lit by hypernovae:<br>Murray 2006.11.21<br><a href="http://groups.yahoo.com/group/AstroDeep/20" rel="nofollow" class="url" target="_blank">http://groups.yahoo.com/group/AstroDeep/20</a><br><br><a href="http://hubblesite.org/newscenter/archive/releases/2004/07/image/b" rel="nofollow" class="url" target="_blank">http://hubblesite.org/newscenter/archive/releases/2004/07/image/b</a>/<br><br><a href="http://imgsrc.hubblesite.org/hu/db/2004/07/images/b/formats/full_tif.tif" rel="nofollow" class="url" target="_blank">http://imgsrc.hubblesite.org/hu/db/2004/07/images/b/formats/full_tif.tif</a><br>7.34 MB tiff<br><br><a href="http://www.flickr.com/photos/rmforall" rel="nofollow" class="url" target="_blank">http://www.flickr.com/photos/rmforall</a>/<br>to access 62 deep sky astrophotos with texts<br><br>#33. Hubble Ultra Deep Field infrared view,<br>brightness +20, and both red and blue colors increased,<br>and green reduced, softness set to 3 of 12 levels, 4.07 MB png,<br>1600X1600 pixels. 4.07 MB png<br><br>The colors have been adjusted to reveal a few faint distant red<br>sources, as well as a background of tiny blue sources, 1-2 pixel size,<br>which are always on the background of dark tangled Murray mesh.<br>Click on All Sizes to view the Original.<br><br><a href="http://static.flickr.com/42/121113050_6b7c705fcb_o.png" rel="nofollow" class="url" target="_blank">static.flickr.com/42/121113050_6b7c705fcb_o.png</a><br><br>The number of the myriad minute blue sources varies noticeably,<br>for instance,from higher south of the bright foreground star,<br>just left of center at the bottom, to lower towards the lower right.<br>This indicates that simple surveys can collect much detailed<br>information. (Use the All Sizes button and select Original.)<br><br>The value of this simple approach is evident,<br>if we take the tiny blue sources to be<br>the earliest massive hypernovae and GRBs,<br>markers that highlight the 3D fractal network distribution of mostly H<br>gas filaments, condensing by gravitational attraction,<br>as the universe bubble continued its expansion.<br>It became cool enough at 380,000 years to allow atoms to form within<br>the former ionized plasma.<br>Transparency emerged from opacity.<br>The intense ultraviolet radiation at 3,000 deg K was redshifted and<br>cooled with the thousand-fold expansion of space-time to<br>comprise our era's Cosmic Microwave Background at just 2.7 deg K,<br>ubiquitious, and uniform to a few parts in a hundred thousand.<br><br>See for yourself, Observer,<br>the deep tapestry of our astrophysical history,<br>hung hugely against the uniform red background<br>downshifted cosmic ultraviolet),<br>the wooly open knit of cooled and condensed H filaments<br>(darkly silhouetting the background),<br>lit like Christmas trees with generations of tiny blue sources,<br>(the downshifted ultraviolet of immense fast-burning, short-lived<br>hypernovae,<br>and a few GRBs,<br>while some twin sources may be the two jet lobes of active galaxies),<br>with vistas of closer and cooler galaxies,<br>ranging from red, orange, yellow, green, blue, and white,<br>from early small clump cluster galaxies to far larger irregular,<br>spiral, and elliptical galaxies,<br>and the little kid in our own neighborhood,<br>the red foreground star with its diffraction spikes<br>from the Hubble Space Telescope,<br>just left of center at the bottom.<br><br><a href="http://arxiv.org/PS_cache/arxiv/pdf/0807/0807.4928v1.pdf" rel="nofollow" class="url" target="_blank">http://arxiv.org/PS_cache/arxiv/pdf/0807/0807.4928v1.pdf</a><br>Protostar Formation in the Early Universe, Naoki Yoshida,<br>Kazuyuki Omukai, Lars Hernquist, Science 2008.08.01 13p<br><br><a href="http://www.physics.uci.edu/Cosmology/Yoshida_Naoki.pdf" rel="nofollow" class="url" target="_blank">http://www.physics.uci.edu/Cosmology/Yoshida_Naoki.pdf</a><br>>From the first stars to the first galaxies, Naoki H Yoshida,<br>27 slides show<br><br><a href="http://online.kitp.ucsb.edu/online/stars_c07/yoshida" rel="nofollow" class="url" target="_blank">http://online.kitp.ucsb.edu/online/stars_c07/yoshida</a>/<br>Second-Generation Star Formation in Proto-Galaxies, Naoki H Yoshida<br>2007.08.17  20 slides show<br><br><a href="http://csaweb.yonsei.ac.kr/~sjyoon/JuniorSeminar/S_and_T/Stars_FirstStar_C2/014" rel="nofollow" class="url" target="_blank">http://csaweb.yonsei.ac.kr/~sjyoon/JuniorSeminar/S_and_T/Stars_FirstStar_C2/014</a>%%<br>5Bbromm%%5Ddark_ages_first_stars.pdf<br>Out of the Dark Ages the First Stars, Volker Bromm,<br>Sky & Telescope, 2006 May, 7 pages pdf<br><br><a href="http://www.space.com/scienceastronomy/080731-first-stars.html" rel="nofollow" class="url" target="_blank">http://www.space.com/scienceastronomy/080731-first-stars.html</a><br>Jeremy Hsu, <a href="http://www.space.com" rel="nofollow" class="url" target="_blank">www.space.com</a> How the first stars were born 2008.07.31<br>____________________________________________________________<br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/bright_blue_1_4_pixel_sources_on_darker_3d_fractal_111062009t.html">no comments</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/bright_blue_1_4_pixel_sources_on_darker_3d_fractal_111062009m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Tue, 05 Aug 2008 09:11:36 PDT</pubDate>
</item>
<item>
	<title><![CDATA[Null Physics?]]></title>
	<guid>http://www.nnseek.com/e/sci.astro.research/null_physics_109291001t.html</guid>
	<link>http://www.nnseek.com/e/sci.astro.research/null_physics_109291001t.html</link>
	<description><![CDATA[Just noticed in the latest Scientific American a 2 page advertisement for a <br>book, "Our Undiscovered Universe" subtitled "Introducing Null Physics". The <br>book has a web site at <a href="http://www.ourundiscovereduniverse.com" rel="nofollow" class="url" target="_blank">www.ourundiscovereduniverse.com</a>.<br><br>I'm no physicist but from looking at that web site- the subject/concept <br>looks flakey. That's OK, there's plenty of flakey scientists and non <br>scientific concepts such as creationism- but they seldom have 2 page <br>advertisements in  Scientific American- so, what's up with this "new" <br>physics? Does it have any respect in the scientific community?<br><br>Joe<br>
    <table border="0" cellspacing="0" cellpadding="0">
      <tr>
        <td width="30">&nbsp;</td>
        <td>Posted In: <a href="http://www.nnseek.com/e/sci.astro.research/">sci.astro.research</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/null_physics_109291001t.html"><b>1</b> Comment</a></td>
        <td width="20">&nbsp;</td>
        <td><a href="http://www.nnseek.com/e/sci.astro.research/null_physics_109291001m.html">Reply</a></td>
      </tr></table><br>]]></description>
	<pubDate>Tue, 22 Jul 2008 02:24:33 PDT</pubDate>
</item>
</channel>
</rss>