2022A&A...668A.124E


Query : 2022A&A...668A.124E

2022A&A...668A.124E - Astronomy and Astrophysics, volume 668A124 (2022/12-1)

How to create Sgr A East Where did the supernova explode?

EHLEROVA S., PALOUS J., MORRIS M.R., WUNSCH R., BARNA B. and VERMOT P.

Abstract (from CDS):

Context. Sgr A East is the supernova remnant closest to the centre of the Milky Way. Its age has been estimated to be either very young, around 1-2 kyr, or about 10 kyr, and its exact origin remains unclear. Aims. We aspire to create a simple model of a supernova explosion that reproduces the shape, size, and location of Sgr A East. Methods. Using a simplified hydrodynamical code, we simulated the evolution of a supernova remnant in the medium around the Galactic centre. The latter consists of a nearby massive molecular cloud with which Sgr A East is known to be interacting and a wind from the nuclear star cluster. Results. Our preferred models of the Sgr A East remnant are compatible with an age of around 10 kyr. We also find suitable solutions for older ages, but not for ages younger than 5 kyr. Our simulations predict that the supernova exploded at a distance of about 3.5 pc from the Galactic centre, below the Galactic plane, slightly eastwards from the centre and 3 pc behind it.

Abstract Copyright: © S. Ehlerová et al. 2022

Journal keyword(s): ISM: supernova remnants - ISM: individual objects: Sgr A East - Galaxy: center

Simbad objects: 9

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Number of rows : 9
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 IC 443 SNR 06 17 00.0000000 +22 34 11.998901           ~ 1314 1
2 NAME Sgr A West HII 17 45 39.4 -29 00 24           ~ 381 0
3 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
4 NAME Galactic Circumnuclear Disk PoG 17 45 40.0 -29 00 28           ~ 187 0
5 GCIRS 16 Cl* 17 45 40.0 -29 00 28           ~ 387 0
6 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 4970 3
7 NAME Sgr A East SNR 17 45 41 -29 00.8           ~ 523 2
8 CXOGC J174545.5-285829 X 17 45 45.52 -28 58 28.5           ~ 30 1
9 [MML2011] G-0.02-0.07 HII 17 45.8 -28 59           ~ 7 0

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