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Welcome to the South Arkansas Astronomical Society. Our intention is to provide astronomical resources and information for schools and interested individuals in the South Arkansas region. If you are interested in an astronomy presentation for your class, or you want to attend the next star party, please feel free to contact us. |
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Astronomer's Telegram - Top Stories |
For reporting and commenting upon new observations of astronomical transients by the professional astrophysics community.
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A spectrum (340-760 nm) of ROTSE3 J133033.0-313427 (Zheng et al., ATel #2468) obtained on Mar 14.58 UT with the 10-m Keck I (+ Low Resolution Imaging Spectrometer) shows it to be a normal Type Ia supernova. ...
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We observed the position of the broad-line Type Ic supernova PTF10bzf (ATel 2470) with the Westerbork Synthesis Radio Telescope at 4.8 GHz, at March 13 17.89 UT to March 14 1.45 UT. ...
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Using 10.1 ks of Swift X-Ray Telescope (XRT) observations of the Type II SN 2008M in ESO 121-026 (CBET #1214), obtained between 2008-01-28 and 2008-01-30, an X-ray point-source is detected at the position of the SN with a 3-sigma significance of source detection. ...
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U Sco is a recurrent nova with a fast decline leveling off to a plateau in the optical light curve (IAUC #9111, ATEL #2452), and it has become visible as a super-soft source (SSS) at the start of the plateau phase (ATEL #2430, ATEL #2442). ...
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MAXI/GSC detected an X-ray transient at the scan transit centered at UT 2010-03-11T02:42:38. The averaged source flux during the scan is about 180 mCrab in the 4-10 keV band. ...
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The Supergiant Fast X-ray Transient (SFXT) IGR J17544-2619 which went to outburst on 2010 March 04 (ATel #2463) was observed in the near-infrared J-band on March 6 and in J, H, and K-band on March 7 with the 1.2m telescope (+ NICS with HAWAII-1 infrared array) at Gurushikhar, Mt Abu, operated by Physical Research Laboratory, Ahmedabad, India. ...
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We report the likely optical ID of the bright transient recently discovered in M31, CXOM31 J004253.1+411422 (Henze et al, ATEL #2356). With a peak X-ray luminosity of nearly 5e39 erg/sec, this is the brightest X-ray transient yet found in M31. ...
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Yahoo News - Astronomy/Astronomical |
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