C.D.S. - SIMBAD4 rel 1.7 - 2021.02.28CET19:42:37

2009A&A...508L..27W - Astronomy and Astrophysics, volume 508, L27-30 (2009/12-3)

Companion stars of type Ia supernovae and hypervelocity stars.

WANG B. and HAN Z.

Abstract (from CDS):

Recent investigations of the white dwarf (WD)+He star channel of Type Ia supernovae (SNe Ia) imply that this channel can produce SNe Ia with short delay times. The companion stars in this channel would survive and potentially be identifiable. In this Letter, we study the properties of the companion stars of this channel at the moment of SN explosion, which can be verified by future observations. According to SN Ia production regions of the WD+He star channel and three formation channels of WD+He star systems, we performed a detailed binary population synthesis study to obtain the properties of the surviving companions. We obtained the distributions of many properties of the companion stars of this channel at the moment of SN explosion. We find that the surviving companion stars have a high spatial velocity (>400km/s) after SN explosion, which could be an alternative origin for hypervelocity stars (HVSs), especially for HVSs such as US 708.

Abstract Copyright:

Journal keyword(s): binaries: general - supernovae: general - stars: evolution - white dwards

Simbad objects: 4

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Number of rows : 4

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
1 HE 0437-5439 HS* 04 38 12.7828185490 -54 33 11.840105637 15.37 16.18 16.42     sdB+F 67 0
2 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 15196 1
3 US 708 HS* 09 33 20.8630614743 +44 17 05.503100302   18.5 18.8     sdOHe 76 0
4 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11996 0

    Equat.    Gal    SGal    Ecl

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