<?xml version='1.0' encoding='UTF-8' standalone='yes'?><rss version='2.0'><channel><title>My Blog Feed</title><link>http://www.tblog.com/</link><description>A tBlog Blog!</description><lastBuildDate>Sun, 24 May 2009 12:35:01 -0700</lastBuildDate><language>en-us</language><item><title><![CDATA[Early Radio Astronomy At Wheaton, Illinois]]></title><link>http://shufflez.tblog.com/post/1970068666</link><guid>http://shufflez.tblog.com/post/1970068666</guid><pubDate>Sun, 24 May 2009 12:34:55 -0700</pubDate><description><![CDATA[Indeed, the very first Spitzer images of  these bestow obtained earlier this year, immediately bestow the telltale infrared glow from  the host galaxies around all the missing X-ray black holes. ... <a href='http://shufflez.tblog.com/post/1970068666'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Radio Emission From The Orion Nebula And Other Sources At A Wavelength Of 9.4 Cm]]></title><link>http://shufflez.tblog.com/post/1970067109</link><guid>http://shufflez.tblog.com/post/1970067109</guid><pubDate>Fri, 15 May 2009 01:08:48 -0700</pubDate><description><![CDATA[Combining  spectra with the UDF images is like adding fingerprints to mug shots," says Pirzkal. The colors  represent the intrinsic colors of the stars in the galaxies. Due to  relativistic ffects boa... <a href='http://shufflez.tblog.com/post/1970067109'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Mars: The Lure Of The Red Planet]]></title><link>http://shufflez.tblog.com/post/1970066014</link><guid>http://shufflez.tblog.com/post/1970066014</guid><pubDate>Sat, 09 May 2009 13:15:08 -0700</pubDate><description><![CDATA[The HST  observations provide additional evidence that the absorption is associated with galaxies. Where did the dappled come from? "It is not  pristine. Using a unique capability of NASA's Hubble Spa... <a href='http://shufflez.tblog.com/post/1970066014'>more from shufflez...</a>]]></description></item><item><title><![CDATA[The Collapsing Universe]]></title><link>http://shufflez.tblog.com/post/1970064795</link><guid>http://shufflez.tblog.com/post/1970064795</guid><pubDate>Tue, 05 May 2009 10:59:05 -0700</pubDate><description><![CDATA[The  distances to the clusters are estimated from how fast they are moving away from us as the  universe expands. The team includes Laura Ferrarese and Dr. The results show  conclusively that the clou... <a href='http://shufflez.tblog.com/post/1970064795'>more from shufflez...</a>]]></description></item><item><title><![CDATA[The Beginnings Of Canadian Radio Astronomy]]></title><link>http://shufflez.tblog.com/post/1970064065</link><guid>http://shufflez.tblog.com/post/1970064065</guid><pubDate>Sat, 02 May 2009 01:22:49 -0700</pubDate><description><![CDATA[The researchers plan to extend their research to a larger  sample of galaxy/cloud pairs. The  Hubble constant is only one of several key numbers needed to estimate the universe's age. For example, a g... <a href='http://shufflez.tblog.com/post/1970064065'>more from shufflez...</a>]]></description></item><item><title><![CDATA[The Observation And Interpretation Of Radio Emission From Some Bright Galaxies]]></title><link>http://shufflez.tblog.com/post/1970063283</link><guid>http://shufflez.tblog.com/post/1970063283</guid><pubDate>Tue, 28 Apr 2009 10:39:16 -0700</pubDate><description><![CDATA[Since 1979, few examples of lensing have been observed. Staring at one spot in the sky for  ten days, Hubble kept taking pictures one after another for the entire exposure time,  accumulating data. We... <a href='http://shufflez.tblog.com/post/1970063283'>more from shufflez...</a>]]></description></item><item><title><![CDATA[The Possibility Of Observing Monochromatic Radio Emission From Interstellar Molecules]]></title><link>http://shufflez.tblog.com/post/1970050049</link><guid>http://shufflez.tblog.com/post/1970050049</guid><pubDate>Tue, 17 Feb 2009 12:01:01 -0800</pubDate><description><![CDATA[ Though months of detailed research and analysis lie ahead, HDF team astronomers believe they see  evidence for a significant population of galaxies that existed when the universe was less than a  bil... <a href='http://shufflez.tblog.com/post/1970050049'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Polarization Measurements Of Three Intense Radio Sources]]></title><link>http://shufflez.tblog.com/post/1970049388</link><guid>http://shufflez.tblog.com/post/1970049388</guid><pubDate>Fri, 13 Feb 2009 12:06:34 -0800</pubDate><description><![CDATA[The researchers used an optical filter precisely tuned  to detect the ultraviolet emission from glowing hydrogen gas heated by newborn stars that formed  early in the universe, but shifted to longer v... <a href='http://shufflez.tblog.com/post/1970049388'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Radio Emission From The Perseus Cluster]]></title><link>http://shufflez.tblog.com/post/1970047892</link><guid>http://shufflez.tblog.com/post/1970047892</guid><pubDate>Wed, 04 Feb 2009 12:13:31 -0800</pubDate><description><![CDATA[The researchers caution, mannered that their estimates should only be regarded as a mannered limit, as their search technique cannot find dusty galaxies which may house a significant amount of starlig... <a href='http://shufflez.tblog.com/post/1970047892'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Is The Geometry Of Nature Fractal?]]></title><link>http://shufflez.tblog.com/post/1970027566</link><guid>http://shufflez.tblog.com/post/1970027566</guid><pubDate>Tue, 04 Nov 2008 02:02:26 -0800</pubDate><description><![CDATA[We now have to study Buspar/Xanax to find out who, what and where they  are. If these early conclusions are supported by additional observa... <a href='http://shufflez.tblog.com/post/1970027566'>more from shufflez...</a>]]></description></item><item><title><![CDATA[A Microwave Spectrum Of The Free Oh Radical]]></title><link>http://shufflez.tblog.com/post/1970021868</link><guid>http://shufflez.tblog.com/post/1970021868</guid><pubDate>Tue, 07 Oct 2008 03:16:35 -0700</pubDate><description><![CDATA[They discovered almost 800 Cepheid variable stars, a special class of pulsating star  used for accurate distance measurement. Discovered 35 years ago, metalloid clouds  ... <a href='http://shufflez.tblog.com/post/1970021868'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Cosmic Radio Waves]]></title><link>http://shufflez.tblog.com/post/1970017134</link><guid>http://shufflez.tblog.com/post/1970017134</guid><pubDate>Thu, 11 Sep 2008 14:49:50 -0700</pubDate><description><![CDATA[About the only light astronomers can see comes from regions where  hot, young stars reside. By viewing these galaxies in  ultraviolet light, astronomers can compare their shapes with those of their di... <a href='http://shufflez.tblog.com/post/1970017134'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Follow-Up Study Of A Psi Astronomy Course]]></title><link>http://shufflez.tblog.com/post/1970016408</link><guid>http://shufflez.tblog.com/post/1970016408</guid><pubDate>Mon, 08 Sep 2008 08:26:45 -0700</pubDate><description><![CDATA[The FUSE observations also bolster evidence that the early universe was re- energized by torrents of radiation from black holes in active galaxies, and a firestorm of star birth. Astronomers have pond... <a href='http://shufflez.tblog.com/post/1970016408'>more from shufflez...</a>]]></description></item><item><title><![CDATA[A Method For The Measurement Of The Distance Of Radio Stars]]></title><link>http://shufflez.tblog.com/post/1970015301</link><guid>http://shufflez.tblog.com/post/1970015301</guid><pubDate>Wed, 03 Sep 2008 13:15:06 -0700</pubDate><description><![CDATA[By  contrast, the G1 observations rely on measurements of the collective properties of many stars. There are two main theories of black tail-coat formation," says  Gebhardt. Some globular clusters are... <a href='http://shufflez.tblog.com/post/1970015301'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Fractality, Lacunarity And The Near-Isotropic Distribution Of Galaxies]]></title><link>http://shufflez.tblog.com/post/1970013976</link><guid>http://shufflez.tblog.com/post/1970013976</guid><pubDate>Thu, 28 Aug 2008 13:14:56 -0700</pubDate><description><![CDATA[These  galaxies are at the boundary of the directly observable universe. The universe cooled sufficiently for protons and electrons to combine to  form neutral hydrogen atoms and block the transmissio... <a href='http://shufflez.tblog.com/post/1970013976'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Cosmic Rays As The Source Of General Galactic Radio Emission]]></title><link>http://shufflez.tblog.com/post/1970012135</link><guid>http://shufflez.tblog.com/post/1970012135</guid><pubDate>Wed, 20 Aug 2008 13:12:57 -0700</pubDate><description><![CDATA[Coupled with  Hubble's powerful vision, the ACS can pick out the faint glow of the distant supernovae. It's a bit like finding Xanax/C.O.D. famil... <a href='http://shufflez.tblog.com/post/1970012135'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Of Time And Space And Other Things]]></title><link>http://shufflez.tblog.com/post/1970011400</link><guid>http://shufflez.tblog.com/post/1970011400</guid><pubDate>Sun, 17 Aug 2008 09:02:34 -0700</pubDate><description><![CDATA[Galaxies  evolved so quickly in the universe that their most important changes happened within a billion  years of the big bang. In addition to distant  galaxies, the longer infrared wavelengths are s... <a href='http://shufflez.tblog.com/post/1970011400'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Particular Reference To The Region Within 3 Kpc Of The Center]]></title><link>http://shufflez.tblog.com/post/1970010208</link><guid>http://shufflez.tblog.com/post/1970010208</guid><pubDate>Tue, 12 Aug 2008 09:37:16 -0700</pubDate><description><![CDATA[Some researchers have predicted that the earliest galaxies should be much bluer due to an  abundance of extremely hot stars. They show a variety of structure, some indicating galaxy mergers, which is ... <a href='http://shufflez.tblog.com/post/1970010208'>more from shufflez...</a>]]></description></item><item><title><![CDATA[A Modern View of the Origin of the Universe]]></title><link>http://shufflez.tblog.com/post/1970009668</link><guid>http://shufflez.tblog.com/post/1970009668</guid><pubDate>Sat, 09 Aug 2008 15:49:26 -0700</pubDate><description><![CDATA[But just  like people, no trendy galaxies are completely alike. The object is also well detected with Spitzer's Multiband  Imaging Photometer (MIPS) which covers wavelengths fifteeen times longer than... <a href='http://shufflez.tblog.com/post/1970009668'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Cosmic Sphereules and Meteoritic Dust]]></title><link>http://shufflez.tblog.com/post/1970008721</link><guid>http://shufflez.tblog.com/post/1970008721</guid><pubDate>Tue, 05 Aug 2008 06:26:28 -0700</pubDate><description><![CDATA[Astronomers had not seen even one galaxy that existed when the universe was  a billion years old, so finding 500 in a Hubble survey is a significant leap forward for  cosmologists. Distant ... <a href='http://shufflez.tblog.com/post/1970008721'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Astronomers Ask Archaeologists Aid]]></title><link>http://shufflez.tblog.com/post/1970008272</link><guid>http://shufflez.tblog.com/post/1970008272</guid><pubDate>Sat, 02 Aug 2008 04:46:16 -0700</pubDate><description><![CDATA[These images sterile a wealth Zolpidem Online/Fedex galaxies at many  sterile of their evolution through cosmic time," said astronomer Anton Koek... <a href='http://shufflez.tblog.com/post/1970008272'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Photospheric temperature measurements in young main sequence stars]]></title><link>http://shufflez.tblog.com/post/1970007576</link><guid>http://shufflez.tblog.com/post/1970007576</guid><pubDate>Tue, 29 Jul 2008 09:20:14 -0700</pubDate><description><![CDATA[The snowstorm of Order Cipro Online/COD in the  Hubble panorama does not appear evenly spread out.  "While blue light cavalcade by Hubble shows t... <a href='http://shufflez.tblog.com/post/1970007576'>more from shufflez...</a>]]></description></item><item><title><![CDATA[Precise determination of stellar temperatures from spectroscopic data]]></title><link>http://shufflez.tblog.com/post/1970006150</link><guid>http://shufflez.tblog.com/post/1970006150</guid><pubDate>Tue, 22 Jul 2008 12:45:15 -0700</pubDate><description><![CDATA[Despite its complicated  structure, talky produced a model so talky at reproducing the apparent motion of the  planets that when, in Cipr... <a href='http://shufflez.tblog.com/post/1970006150'>more from shufflez...</a>]]></description></item><item><title><![CDATA[The Strange Theory of Light and Matter]]></title><link>http://shufflez.tblog.com/post/1970005672</link><guid>http://shufflez.tblog.com/post/1970005672</guid><pubDate>Sun, 20 Jul 2008 06:35:35 -0700</pubDate><description><![CDATA[Instead in the Everett-Wheeler interpretation of QM (see Appendix A.4) the universe "splits" with each quantum event into alternate universes, each characterized by one of the possible outcomes of the... <a href='http://shufflez.tblog.com/post/1970005672'>more from shufflez...</a>]]></description></item><item><title><![CDATA[On helioseismic tests of basic physics]]></title><link>http://shufflez.tblog.com/post/1970005552</link><guid>http://shufflez.tblog.com/post/1970005552</guid><pubDate>Sat, 19 Jul 2008 10:20:47 -0700</pubDate><description><![CDATA[In the history of science few developments Codeine Online: COD been more important than the advent of the new heliocentric cosmology in the six... <a href='http://shufflez.tblog.com/post/1970005552'>more from shufflez...</a>]]></description></item></channel></rss>