2011CBET.2946....2M


Query : 2011CBET.2946....2M

2011CBET.2946....2M - Central Bureau Electronic Telegrams, 2946, 2 (2011/December-0)

Supernova 2011ja in NGC 4945 = PSN J13051112-4931270.

MILISAVLJEVIC D., FESEN R., PICKERING T., ROMERO-COLMENERO E., SODEBERG A. and MARGUTTI R.

Abstract (from CDS):

D. Milisavljevic, Harvard-Smithsonian Center for Astrophysics (CfA); R. Fesen, Dartmouth College; T. Pickering and E. Romero-Colmenero, South African Astronomical Observatory and Southern African Large Telescope; and Alicia Soderberg and Raffaella Margutti, CfA, report that low-dispersion spectra (range 350-880 nm), obtained on Dec. 19.1 UT during morning twilight with the 10-m SALT telescope (+ RSS), show PSN J13051112-4931270 = SN 2011ja to be a relatively young type-II supernova. Cross-correlation with a library of supernova spectra using the "Supernova Identification" code (SNID; Blondin and Tonry 2007, Ap.J. 666, 1024) shows a reasonable match to the type-IIP event SN 2004et about a week after maximum light. After removal of the host-galaxy recession velocity of 460 km/s (determined from narrow emission lines), the absorption minimum of the H-alpha line is found to be blueshifted by about -11000 km/s. A suppressed blue continuum and noticeable absorption around Na I are suggestive of significant internal extinction.

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 SN 2011ja SN* 13 05 11.12 -49 31 27.0           SNIIP 48 0

Query : 2011CBET.2946....2M

Basic data :
SN 2011ja -- SuperNova
Other object types:
otypes_help
SN* (SN), SN? (PSN)
ICRS coord. (ep=J2000) :
13 05 11.12 -49 31 27.0 [ ] B 2011CBET.2946....1M
FK4 coord. (ep=B1950 eq=1950) :
13 02 15.97 -49 15 23.0 [ ]
Gal coord. (ep=J2000) :
305.22348 +13.28640 [ ]
Spectral type:
SNIIP C 2015MNRAS.452.2597X
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Identifiers (2) :
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SN 2011ja PSN J13051112-4931270

References (48 between 1850 and 2026) (Total 48)
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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