[vsnet-outburst 10810] V406 Hya outburst and SDSS J012940.05+384210.4
Taichi Kato
tkato at kusastro.kyoto-u.ac.jp
Sun Dec 6 13:36:45 JST 2009
According to ATEL, V406 Hya (= SN2003aw) is also in outburst.
This object also showed multiple rebrightenings similar to those of EG Cnc
during the 2004 superoutburst:
http://adsabs.harvard.edu/abs/2004PASJ...56L..39N
The detection of SDSS J012940.05+384210.4 on Dec. 3 clearly spotted
the rising stage of the "rebrightening" detected by Maehara-san.
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The Astronomer's Telegram http://www.astronomerstelegram.org
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ATEL #2334 ATEL #2334
Title: Two AM CVn systems in outburst - V406 Hya and SDSS J0129+3842
Author: T. Barclay (Armagh Observatory/MSSL-UCL), G. Ramsay (Armagh
Observatory), D. Steeghs (Warwick), P. Wheatley (Warwick), S. Rosen
(Leicester)
Queries: tsb at arm.ac.uk
Posted: 5 Dec 2009; 17:26 UT
Subjects: Request for Observations, Binaries, Cataclysmic Variables,
Novae, Variables
We are conducting a campaign of monitoring AM CVn systems visible from
the Northern Hemisphere once a week using the Liverpool Telescope on La
Palma. On the night of 3/4 December 2009 we observed two of the AM
CVn systems to be in a state of outburst, V406 Hya (RA=09:05:54.79, Dec=-05:36:08.6)
and SDSS J0129+3842 (RA=01:29:40.06, Dec=+38:42:10.4). V406 Hya (also known
as 2003aw) has a typical quiescent brightness of g~20.2. At 02:21UT we
observed this system at a g magnitude of 14.80+-0.02. We observed
SDSS J0129+3842 to be at g=16.81+-0.02 at 22:58UT, 3.2 mag. brighter than
the typical quiescent brightness of g~20.05+-0.05. We observed this system
again a day later at 22:28UT on 4 December 2009 at a brightness of g=15.13+-0.02.
Both these outbursts are above ~5 magnitudes and are among the highest
amplitude outbursts observed in AM CVn systems. Our observations are continuing
and we encourage further observations.
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