2008ApJ...685.1103W

Query : 2008ApJ...685.1103W

2008ApJ...685.1103W - Astrophys. J., 685, 1103-1108 (2008/October-1)

The most massive core-collapse supernova progenitors.

WALDMAN R.

Abstract (from CDS):

The discovery of the extremely luminous supernova SN 2006gy, possibly interpreted as a pair instability supernova, renewed the interest in very massive stars. We explore the evolution of these objects, which end their life as pair instability supernovae or as core-collapse supernovae with relatively massive iron cores, up to about 3 M☉.

Abstract Copyright: ∼

Journal keyword(s): Stars: Evolution - Stars: Supernovae: General

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 2006gy SN* 03 17 27.06 +41 24 19.5       14.20   SNIIn 372 1

Query : 2008ApJ...685.1103W

Basic data :
SN 2006gy -- SuperNova
Other object types: otypes_help 		SN* (2012A&A,SN)
ICRS coord. (ep=J2000) : 		03 17 27.06 +41 24 19.5 [ ] D 2006IAUC.8754....1F
FK4 coord. (ep=B1950 eq=1950) : 		03 14 09.03 +41 13 21.4 [ ]
Gal coord. (ep=J2000) : 		150.25681 -13.59159 [ ]
Radial velocity / Redshift / cz : 		V(km/s) 5642 [~] / z(~) 0.019 [~] / cz 5696 [~]
   D 2012Sci...337..927G
Spectral type: 		SNIIn C 2008yCat....1.2024B
Fluxes (1) :
R 14.20 [~] D 2008yCat.2283....0B
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SN 2006gy

References (372 between 1850 and 2026) (Total 372)
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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