2001ApJ...560L..83M


Query : 2001ApJ...560L..83M

2001ApJ...560L..83M - Astrophys. J., 560, L83-L86 (2001/October-2)

The origin of the Local Bubble.

MAIZ-APELLANIZ J.

Abstract (from CDS):

The Sun is located in a low-density region of the interstellar medium partially filled with hot gas that is the likely result of several nearby supernova explosions within the last 10 Myr. Here we use astrometric data to show that part of the Scorpius-Centaurus OB association was located closer to the present position of the Sun 5-7 Myr ago than today. Evolutionary synthesis models indicate that the association must have experienced ∼20 supernova explosions in the last 10-12 Myr, a prediction that is supported by the detection of four or five runaway stars escaping from it. The approximately six supernovae produced by the Lower Centaurus Crux subgroup are likely responsible for the creation of the Local Bubble.

Abstract Copyright: ∼

Journal keyword(s): ISM: Bubbles - ISM: Structure - open clusters and associations: individual (Scorpius-Centaurus Association) - Galaxy: Solar Neighborhood - Stars: Distances - Stars: Supernovae: Individual: Name: Scorpius-Centaurus Association

Simbad objects: 11

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Number of rows : 11
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 NAME Lower Centaurus Crux As* 12 19 -57.1           ~ 565 1
2 NAME NGP reg 12 51 26.275 +27 07 41.70           ~ 1274 0
3 NAME Loop I SR? 15 01 -38.7           ~ 414 2
4 NAME Upper Centaurus Lupus MGr 15 24 -41.9           ~ 567 1
5 NAME Upper Sco Association As* 16 12 -23.4           ~ 1586 1
6 NAME Upper Sco-Cen As* 16 15 -24.2           ~ 1497 1
7 NAME Oph Cloud Complex DNe 16 30 -24.3           ~ 67 1
8 * zet Oph Be* 16 37 09.5400587698 -10 34 01.509742704 1.73 2.58 2.56 2.46 2.50 O9.2IVnn 1908 0
9 NAME Aql Rift DNe 18 32 -01.0           ~ 355 1
10 PSR B1929+10 Psr 19 32 14.0570 +10 59 33.380           ~ 801 0
11 NAME Local Bubble ISM ~ ~           ~ 1059 0

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