(cba:news) [Fwd: ATel 1867]
Joe Patterson
jop at astro.columbia.edu
Mon Dec 8 10:02:58 EST 2008
Dear CBAers,
Given the amplitude of this dwarf nova, it may very well be one of our
favorites - in the WZ Sge class. Andromeda is not very well positioned
now... and the background galaxy might be pretty annoying... but see if
you can get a time series on it, while it's still bright (if it is).
We can still solve for a unique period, if we get a USA-Europe baseline.
Here's the 2000 position:
00 42 26.50 +42 15 36.7
Sorry if it's a bad field. Here in New York, I dunno!
joe
-------- Original Message --------
Subject: ATel 1867
Date: Mon, 8 Dec 2008 01:41:50 -0500 (EST)
From: atel at astronomerstelegram.org
To: jop at astro.columbia.edu
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The Astronomer's Telegram
http://www.astronomerstelegram.org
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Posted: Sun Dec 7 01:30:01 EST 2008 -- Mon Dec 8 01:30:02 EST 2008
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ATEL #1867 ATEL #1867
Title: M31N2008-11b is a Galactic Dwarf Nova
Author: M. M. Kasliwal, R. Quimby, S. R. Kulkarni (Caltech)
Queries: mansi at astro.caltech.edu
Posted: 8 Dec 2008; 4:28 UT
Subjects: Cataclysmic Variables, Novae, Transients, Variables
We observed M31N2008-11b <a
href='http://www.cfa.harvard.edu/iau/CBAT_M31.html#2008-11b'>(K.
Itagaki, CBET#1588)</a> with the Double Beam Spectrograph on the Palomar
Hale 5-m telescope on UT Dec 4.221. This spectrum has a steep blue
continuum,
very narrow emission in H-alpha and broad absorption in H-beta through
at least H-eta. Further, there is a faint blue counterpart in SDSS DR
Supplement
g-band imaging (g=22.8, r > 23.3). Given the reported peak magnitude of
14.5 (CBET#1588), this outburst had an amplitude of >8 mag. We suggest
that this optical transient is an SU-UMa-like superoutburst in our own
galaxy similar to HS2219+1824 (Rodriguez-Gil et al 2005).
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Password Certification: Mansi Manoj Kasliwal (mansi at astro.caltech.edu)
http://www.astronomerstelegram.org/?read=1867
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Events, Neutron Stars, Novae, Planets, Planets (minor), Pulsars, Quasars,
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