2009CBET.2015....3K

Query : 2009CBET.2015....3K

2009CBET.2015....3K - Central Bureau Electronic Telegrams, 2015, 3 (2009/November-0)

Possible recurrent nova in M31: M31N 2009-11b.

KASLIWAL M.M.

Abstract (from CDS):

M. M. Kasliwal et al. (http://www.astronomerstelegram.org/?read=2290) report that observations obtained of 2009-11b with the Double Beam Spectrograph at the Palomar 5-m telescope on Nov. 8.35 UT yields a spectrum that shows prominent Balmer emission from H-alpha through H-delta; the emission peaks are blue-shifted by about 360 km/s, which is consistent with M31. The Gaussian FWHM of the H-alpha line is about 1280 km/s. Also, H-beta, H-gamma, and H-delta show P-Cyg profiles. This suggests that 2009-11b is a recurrent nova in M31.

Abstract Copyright: ∼

Journal keyword(s):

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 AT 2021vgi No* 00 42 39.59 +41 09 04.0           ~ 22 0

Query : 2009CBET.2015....3K

Basic data :
AT 2021vgi -- Classical Nova
Other object types: otypes_help 		SN* (), No* (2007A&A,M31N,...), ev (AT,PTF), No? (2021ATel14842)
ICRS coord. (ep=J2000) : 		00 42 39.59 +41 09 04.0 [ ] B 2009CBET.2015....1N
FK4 coord. (ep=B1950 eq=1950) : 		00 39 55.42 +40 52 38.2 [ ]
Gal coord. (ep=J2000) : 		121.15374 -21.69033 [ ]
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1 : 26745 Display criteria :

Identifiers (7) :
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AT 2021vgi M31N 2021-08a M31N 2001-12b [PFF2005] WeCAPP-N2001-15
M31N 2009-11b M31N 1997-11k PTF 09gfq

References (22 between 1850 and 2026) (Total 22)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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