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1. Supernova 2002ao in UGC 9299
Supernova 2002ao in UGC 9299 . This page is devoted to information on Supernova 2002ao in UGC 9299 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. ... AAVSO has a 2002ao page . ... VSNET 2002ao summary page . ... vsnet-campaign-sn 326] SN 2002ao in UGC 9299 . ... vsnet-campaign-sn 339] Re: SN 2002ao in UGC 9299 . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/sn2002/sn2002ao.html -- 9.2 Кб -- 22.12.2007
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/sn2002/sn2002ao.html -- 9.2 Кб -- 19.04.2014
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2. SAI Supernova catalog
... Initially SAI Supernova Catalogue was presented in the form of filebased system. ... The current version of SAI Supernova Catalogue presents data on supernovae together with data on their parent galaxies. ... The main source of data for the galaxies was LEDA database. ... In some cases our data were compared with the ones from the Asiago Supernova Catalogue and from List of Supernovae at Harvard-Smithsonian Center for Astrophysics, but the compilation of our Catalogue is carried out independently. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/sn/sncat/ -- 5.9 Кб -- 04.02.2013
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3. How do galaxies form? - New discovery from European Southern Observatory |
Astronotes Armagh Planetarium's Stellar Blog! ... Our Galaxy . ... Stars . ... Space Flight . ... A galaxy is born: This artist's impression shows a young galaxy, about two billion years after the Big Bang, accreting material from the surrounding hydrogen and helium gas and forming many young stars. ... Galaxies, distant from us in space and time, have been in the news recently. ... Astronomers at the European Southern Observatory have observed another process which helped primordial galaxies grow. ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/another-galaxy-far-far-away-seen-by-hst-and-eso.html -- 42.6 Кб -- 09.04.2016
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4. Supernova Remnant (SNR) Catalogue or Catalog of Galactic SNRs
2014 May version . ... Green D. A., 2014 , Bulletin of the Astronomical Society of India, 42 , 47-58. ( .pdf , or arXiv.org:1409.0637 ) If you make use of the detailed version of the catalogue, then plaese also cite: . Green D. A., 2014, `A Catalogue of Galactic Supernova Remnants (2014 May version)' , Cavendish Laboratory, Cambridge, United Kingdom (available at "http://www.mrao.cam.ac.uk/surveys/snrs/" ). ... Copyright D. A. Green 2014. 25872nd access to this version of the catalogue. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/surveys/snrs/ -- 8.1 Кб -- 09.04.2016
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5. Keep Us Informed - an Astronomy Net Eyepieces Forum Message
Eyepieces Forum Message . Forums: . ... Discussion Forums | ... Post . ... Keep Us Informed . ... Post Message | ... Posted by L Madia on October 17, 2003 16:43:57 UTC . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/eyepieces/messages/475.shtml -- 13.1 Кб -- 09.04.2016
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6. Why do Radiopulsars not Usually Form Pairs with Normal Stars?
Next: Caverns in Binary Systems Up: Ejectors in Massive Binary Previous: The Number of Ejectors . In the very first years after the discovery of radiopulsars, it became clear that for some reason they avoid forming binary systems. ... Illarionov and Sunyaev (1975)[ 76 ] noted the fact that coherent radiowaves with a wavelength longer than 75 cm, which make it possible to observe most of the radiopulsars, are absorbed effectively in the stellar wind of a normal star. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node54.html -- 7.3 Кб -- 26.02.1997
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7. ESO - Thesis Topic: Discovery and characterisation of Pre Main Sequence stars
... Southern . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Discovery and characterisation of Pre Main Sequence stars in southern star forming regions . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Using a robust method to identify Pre-Main Sequence (PMS) stars through their photometric excess in the Hн± band, we have recently studied the star formation history in several star burst clusters in the Galaxy, Small and Large Magellanic Clouds. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/activities/thesis-topics/abstr-gbeccari.html -- 29.2 Кб -- 10.04.2016
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8. Watch Galaxies Form
Astronomy Picture of the Day . ... 5.09.1996 . ... They found many merging groups of stars and gas which have been dubbed "pre-galactic blobs." A particularly dense bunch of these small blue merging objects are visible in the above picture. ... This adds evidence that galaxies formed from the conglomeration of smaller objects instead of the fragmentation of larger objects . ... September 1996 . ... NASA Web Site Statements, Warnings, and Disclaimers . ... U. Based on Astronomy Picture Of the Day ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1160087 -- 13.3 Кб -- 22.04.2003
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9. Detection of a Massive Dust Shell around the Type II Supernova SN 2002hh
Dust emission from the Type II supernova SN 2002hh in NGC 6946 has been detected at mid-infrared wavelengths by the Spitzer Space Telescope from 590 to 758 days after outburst and confirmed by higher angular resolution Gemini North mid-IR observations. ... The minimum emitting radius of 1.1У?1017 cm is too large for the emitting dust to have been formed in the supernova ejecta. ... ADS Citation Query . citations = 25 . ... 2006,6][2007,4][2008,2][2009,4][2010,2][2011,3][2012,1][2013,2][2015,1] . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2005ApJ...627L.113B.html -- 4.1 Кб -- 21.01.2016
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10. Molecular Lines in Starburst Galaxies
... The molecular lines group at Arecibo Observatory consists of Chris Salter, Tapasi Ghosh and Robert Minchin. ... The molecular line group at Arecibo Observatory started in 2006 with a proposal to carry out a spectral census of the star-burst galaxy Arp 220 . ... However, the most interesting discovery came from the observations of the polar ring galaxy, NGC 660. ... Molecular Lines in NGC 660 Arias de Saavedra Benitez et al., ... A cm-Wavelength Search for Pre-Biotic Molecules in Starburst Galaxies. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~rminchin/mol_lines.shtml -- 9.6 Кб -- 09.04.2016
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11. Life from Mars: The Discovery
Life from Mars: . The Discovery . ... Meteorite Yields Evidence of Primitive Life on Early Mars (August 7, 1996) . Life from Mars: Video Animations . ... The NASA-funded team found the first organic molecules thought to be of Martian origin; several mineral features characteristic of biological activity; and possible microscopic fossils of primitive, bacteria-like organisms inside of an ancient Martian rock that fell to Earth as a meteorite. ... Mars Life? Microscopic Structures . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/solar/eng/marslif1.htm -- 10.1 Кб -- 15.10.1997
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/marslif1.htm -- 11.1 Кб -- 15.03.1998
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12. The High-Z SN Search Description
... It turns out one possibility is a form of matter/energy invented by Einstein in the 1920s to make sure his equations of General Relativity did not predict the Expansion of the Universe. Although Einstein was willing to predict several things with his equations of General Relativity, he obviously thought an expanding Universe was too much, and so he invented the Cosmological Constant, which repels itself, and was meant to balance the force of gravity, and make the Universe static. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~brian/PUBLIC/data.html -- 9.6 Кб -- 01.10.2012
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13. ASP: An Ancient Universe - The Age of the Chemical Elements
An Ancient Universe: How Astronomers Know the Vast Scale of Cosmic Time . ... d) The Age of the Chemical Elements . ... Some isotopes (forms of the element with different numbers of neutrons in the nucleus) of these elements are radioactive; they change into other isotopes at a rate that can be measured accurately in the laboratory. ... The Ancient Universe - The Age of the Expanding Universe - The Age of the Oldest Stars - The Age of Light From Distant Galaxies - The Age of the Chemical Elements | ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/publications/tnl/56/ancient4.html -- 8.8 Кб -- 02.10.2012
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14. Forming of supernova explained | Astronomy.com
... Observing . ... Forming of supernova explained . White dwarf "sibling rivalry" exploded into supernova. ... Supernova 2006gz, marked in this photo, shows the strongest evidence yet that it was caused by the merger of two white dwarfs. ... A stronomers at the Harvard-Smithsonian Center for Astrophysics (CfA) have found that a supernova discovered last year was formed when two white dwarf stars collided. ... Only registered members of Astronomy.com are allowed to comment on this article. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/news/2007/11/forming-of-supernova-explained -- 70.2 Кб -- 10.04.2016
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15. Astronaut Bio: Bruce McCandless II
National Aeronautics and Space Administration . ... Bruce McCandless II (Captain, USN, Ret.) NASA Astronaut (former) . ... He was a member of the astronaut support crew for the Apollo 14 mission and was backup pilot for the first manned Skylab mission (SL-1/SL-2). ... A veteran of two space flights, McCandless has logged over 312 hours in space, including 4 hours of MMU flight time. ... With the completion of this flight McCandless logged 191 hours in space (including 4 hours of MMU flight time). ...
[ Сохраненная копия ]  Ссылки http://www.jsc.nasa.gov/Bios/htmlbios/mccandless-b.html -- 9.2 Кб -- 07.07.2015
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16. SNRs Spectra Request Form
Input the SNRs name (Glll.l+-bb.b) . ... possible SNR): G000.0+0.0 G004.5+6.8 G007.7-3.7 G012.2-1.1 G018.8+ 0.3 G027.4+0.0 G000.3+0.0 G004.7+1.3 G008.7-0.1 G013.5+ 0.2 G018.9-1.1 G027.8+ 0.6 G000.9+ 0.1 G004.8+6.2 G008.7-5.0 G015.1-1.6 G020.0-0.2 G029.7-0.3 G001.0-0.1 G005.2-2.6 G009.7-0.1 G015.9+ 0.2 G021.5-0.9 G030.7+ 1.0 G001.4-0.1 G005.4-1.2 G009.8+ 0.6 G016.0+2.7 G021.8-0.6 G030.7-2.0 G001.9+ 0.3 G005.9+3.1 G010.0-0.3 G016.2-2.7 G022.7-0.2 G031.5-0.6 G003.2-5.2 G006.1+ ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/snr_spectra.html -- 5.0 Кб -- 06.05.2008
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18. http://www.asc.rssi.ru/RadioAstron/meetings/telecon/mar16_2011.pdf
MINUTES of the RadioAstron Teleconference on March 16, 2011 N. Kardashev chaired the teleconference. ... He confirmed the priority status of the mission with the launch date scheduled for late June 2011. ... N. Kardashev reminded the participants to send their willing to visit the launch site to M. Lisakov not later than March 20 2011. ... New Zeland JIVE, The Netherlands ASC, Russia NRAO, USA NRAO, USA ASC, Russia NRAO, USA ASC, Russia MPIfR, Germany ASC, Russia NRAO, USA ...
[ Текст ]  Ссылки http://www.asc.rssi.ru/RadioAstron/meetings/telecon/mar16_2011.pdf -- 38.8 Кб -- 15.06.2011
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19. IRAS01005+7910
... The variability of the spectrum of the optical component of the IR-source IRAS01005+7910 was discovered for the first time in the BTA spectra [1]. ... The spectral features include absorptions that form in near-photospheric layers, narrow envelope emissions, and emission-absorption profiles that form in photosphere-to-envelope transition layers (the wind). ... Discovery of spectral variation in the optical counterpart of IRAS01005+7910. ... Dashed line - envelope curve of all the SiII 5979 profiles ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2014/Klochkova2/ -- 6.1 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2014/Klochkova2/ -- 6.1 Кб -- 10.04.2016
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20. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ArtistтАЩs impressions of the surface of HE2359-2844. ... An alien observer close to the star might be able to see the lead- and zirconium-rich cloud layers using specially chosen filters. ... Hot subdwarfs represent a group of low-mass helium-burning stars formed through binary- star interactions and include some of the most chemically peculiar stars in the Galaxy. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2013/638.html -- 6.3 Кб -- 11.03.2014
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