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Query : 1998A&A...333..557D |
1998A&A...333..557D - Astronomy and Astrophysics, volume 333, 557-564 (1998/5-2)
The relative frequency of type II and Ib,c supernovae and the birth rate of double compact star binaries.
DE DONDER E. and VANBEVEREN D.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): stars: binaries - stars: supernovae: general - stars: pulsars: general - black hole physics
Simbad objects: 1
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 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | V* BP Cru | HXB | 12 26 37.5605188992 | -62 46 13.261044684 | 12.482 | 10.803 | 10.304 | B1Ia+ | 689 | 0 |
Query : 1998A&A...333..557D |
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The link on the acronym of the identifiers give access to the
information for this acronym in the dictionary of nomenclature.
Identifiers (43) :
|
4U 1223-624 | INTREF 497 | SWIFT J122637.3-624610 | WISE J122637.57-624613.2 |
3A 1223-624 | 1M 1223-624 | 1SXPS J122637.1-624610 | WRAY 15-977 |
GPS 1222-625 | 2MASS J12263756-6246132 | TIC 450572050 | 1XRS 12238-624 |
GSC 08979-01108 | MO 1-3 | TYC 8979-1108-1 | [BM83] X1223-624 |
GX 301-02 | MSX6C G300.0980-00.0351 | 2U 1223-62 | [GM76] 40 |
GX 301+00 | PBC J1226.6-6246 | 3U 1223-62 | [KRL2007b] 116 |
GX 301-00.2 | 2S 1223-624 | 4U 1223-62 | AAVSO 1221-62 |
1H 1221-623 | SBC9 724 | UCAC2 4126327 | Gaia DR3 6054569565614460800 |
Hen 3-788 | SSTGLMC G300.0981-00.0352 | UCAC4 137-083467 | Gaia DR1 6054569561285282304 |
H 1223-624 | SWIFT J1226.6-6244 | V* BP Cru | Gaia DR2 6054569565614460800 |
INTEGRAL1 10 | SWIFT J1226.6-6246 | WEB 10801 |
References (689 between 1850 and 2024) (Total 689)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). Follow new references on this object |
Observing logs
Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center
Data at NED - NASA/IPAC Extragalactic Database : V* BP Cru
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