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1. Supernova 2011iv in NGC 1404
Supernova 2011iv in NGC 1404 . This page is devoted to information on 2011iv in NGC 1404 . 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 links web page. ... We have a Photometry reference image made by Odd Trondal. This supernova is in the Constellation Eridanus . ... 2011/12/02.570 . ... Joseph Brimacombe . ... 12.4 . ...
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/sn2011/sn2011iv.html -- 8.4 Кб -- 03.07.2014
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2. Bright Supernova in M82
Astronomy Picture of the Day . Bright Supernova in M82 . ... But in this image taken January 23rd , an arrow does point to an exciting, new supernova , now cataloged as SN 2014J, in nearby bright galaxy M82. ... Spectra indicate it is a Type Ia supernova caused by the explosion of a white dwarf accreting matter from a companion star. ... Publications with keywords: starburst galaxy - star formation - supernova . Publications with words: starburst galaxy - star formation - supernova . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1299022 -- 15.8 Кб -- 24.01.2014
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3. Supernova 2011iv in NGC 1404
Supernova 2011iv in NGC 1404 . This page is devoted to information on 2011iv in NGC 1404 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . ... This supernova is in the Constellation Eridanus . ... AAVSO 2011iv in Eridanus in Spanish [ Translate ] . ... 2011/12/02.570 . ... 2011/12/03.024 . ... 2011/12/04.320 . ... 2011/12/04.491 . ... 2011/12/04.508 . ... Joseph Brimacombe . ... 12.4 . ... 2011/12/13 . ... Stan Howerton . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/sn2011/sn2011iv.html -- 8.0 Кб -- 05.02.2013
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4. APOD: February 9, 1999 - A Supernova Starfield
... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. February 9, 1999 . A Supernova Star-Field . Credit: Hubble Heritage Team ( AURA / STScI / NASA ) . Explanation: Bright stars don't last forever. ... The above picture is a composite of recent images taken over several years. The explosion originated from a bright massive star that ran out of nuclear fuel . ... About APOD > . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap990209.html -- 4.5 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/sn1987a_heritage_big.html -- 4.4 Кб -- 02.02.2001
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5. Dust in the bright supernova remnant N49 in the LMC
We investigate the dust associated with the supernova remnant (SNR) N49 in the Large Magellanic Cloud (LMC) as observed with the Herschel Space Observatory. N49 is unusually bright because of an interaction with a molecular cloud along its eastern edge. We have used PACS and SPIRE to measure the far IR flux densities of the entire SNR and of a bright region on the eastern edge of the SNR where the SNR shock is encountering the molecular cloud. ... ADS Citation Query . citations = 21 . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2010A&A...518L.139O.html -- 4.7 Кб -- 21.01.2016
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6. Galaxy Gallery Page II
... They cover a period of 4 days in which the Supernova continues to rise in brightness (what astronomers call magntiude). ... First Image Taken on March 11 at 8:22 UT. Second Image Taken on March 12 at 8:52 UT. ... The supernova is the same brightness as in the previous image taken 2 hours ago . ... This image, taken 24 hours after the previous image, shows the supernova to be another 0.21mag (or about 25%) brighter. ... Hopefully the images do show that the brightness of the Supernova is changing. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/sn.html -- 6.3 Кб -- 07.10.1996
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7. Supernova in the Cigar Galaxy | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Colin Johnston . ... Our Galaxy . ... To locate it, look along the imaginary line between the two end stars on the leading edge of the PloughтАЩs blade (Merak and Dubhe) and Polaris (the North Star), the galaxy M82 (also known as the Cigar Galaxy) along with its companion M81, lies just off this line about a third of the way between the Plough and Polaris. €а€аAs usual, the supernova is far brighter than its home galaxy, appearing as an extra star. ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/supernova-in-the-cigar-galaxy.html -- 43.6 Кб -- 09.04.2016
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8. The Parkes 6 cm Galactic Survey
... 1Haynes+ A catalogue at 5 GHz of 915 sources in the Galactic plane is presented. Sources with a peak beam brightness temperature of at least 0.2 K above the surrounding background are included, except in confused regions; a point source of 0.2 K corresconds to 0.26 Jy. ... It was assumed that Hydra A was a point source with a peak flux density of 13 Jy at 5 GHz; this is equivalent to a mean beam brightness temperature of 10.0 K for a beamwidth of 4.1x4.4'. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/PKSGAL.html -- 6.0 Кб -- 18.03.2015
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9. Bright prospects: Comparing the H Survey with large-scale radio continuum
... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Australia Telescope 20GHz Survey . ... Bright prospects: Comparing the H Survey with large-scale radio continuum emission . ... Prospects for comparisons between the AAO/UKST H \ survey and large-scale radio continuum emission are considered, with particular reference to the recently completed Parkes 2.4-GHz survey of the southern Galactic Plane. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/duncan/paper/index.html -- 52.4 Кб -- 08.04.2016
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