AAVSO Newsletter 51 is now online
AAVSO Newsletter 51, January 2012, is now online.
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AAVSO Newsletter 51, January 2012, is now online.
There are over 100 new and revised charts and sequences since the last update in November. Many of these are for stars in the newly formed YSO Section Program, southern stars with new photometry from APASS and campaign targets. The rest are revisions based on issues reported to CHET and requests for new sequences from our observers.
January 27, 2012: The symbiotic variable RT Cru has brightened in hard x-rays. Dr. Jeno Sokoloski, Columbia University, has requested AAVSO assistance in monitoring RT Cru both now and in the future to see if it is doing anything unusual in the optical. The Swift/BAT hard X-ray light curve shows RT Cru has apparently been gradually brightening over the past few years.
The Norwich Bulletin, of Norwich, Ct., published an article about AAVSO co-founder William Tyler Olcott in their blog focused on the history of the town. It includes interesting tidbits about Mr. Olcott, references to the AAVSO and proposals for ways to commemorate him.
Various AAVSO staff will be in the AAVSO Chat Room on Thursday, January 26. Stop by to chat with other AAVSOers and staff.
Thanks to the hard work, dedication, and persistence(!) of AAVSO member/observer Péter Molnár and Dr. László Kiss, the January 2010 edition of the "Manual for Visual Observing of Variable Stars" is now available in Hungarian.
http://www.aavso.org/visual-observing-manual-hungarian
If you know of anyone who may benefit from this translation, please spread the word!
January 21, 2012: In IAU Central Bureau Electronic Telegram 2974 (Daniel W. E. Green, ed.), B. Moore, J. Newton, and T. Puckett report the discovery of an apparent supernova in the irregular galaxay NGC 3239 at unfiltered magnitude 14.6 taken with a 0.40-m reflector at Portal, AZ, on 2012 Jan. 7.3869 UT in the course of the Puckett Observatory Supernova Search. SN 2012A was confirmed by Puckett at magnitude 14.4 on Jan. 8.3352; nothing is visible down to magnitude 19.0 on his images from 2011 Dec. 29.
ej153: New Light Curve for the 1909 Outburst of RT Serpentis
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