2001A&A...367..613O


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.04CEST22:00:16

2001A&A...367..613O - Astronomy and Astrophysics, volume 367, 613-616 (2001/2-4)

An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105.

OSTROWSKI M. and FUERST E.

Abstract (from CDS):

The energy ejected from the galaxy micro-quasar GRS 1915+105 in the form of jets is expected to lead to formation of an extended double lobe/hot-spot structure with an energy content comparable to an average supernova remnant. We used the Effelsberg 100m telescope at 10.45GHz in attempt to identify such structures. For this distant galactic plane source, no definite identification was possible, due to high confusion by numerous background sources; however, a few suspect structures were identified.

Abstract Copyright:

Journal keyword(s): ISM: jets and outflows - shock waves - acceleration of particles - radio continum: ISM

Nomenclature: Fig.2: [OF2001] A (Nos A-C).

CDS comments: GRS 1915+105 = Granat 1915+105.

Simbad objects: 12

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Number of rows : 12

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 V* BR Cir HXB 15 20 40.85 -57 10 00.1   21.4 21.4     ~ 721 1
2 V* V818 Sco LXB 16 19 55.0688745859 -15 38 25.019920749 11.60 12.40 11.1     Oev 1525 0
3 SS 433 HXB 19 11 49.5645897701 +04 58 57.824087535   16.3 13.0     A7Ib: 1928 3
4 Caswell OH 045.12+00.13 HII 19 13 27.845 +10 53 36.74           ~ 111 0
5 [OF2001] C Rad 19 14 +11.5           ~ 1 0
6 [CKW87] 191147.3+110702 HII 19 14 08.5 +11 12 16           ~ 26 0
7 IRAS 19124+1106 IR 19 14 45 +11 12.1           ~ 22 0
8 Granat 1915+105 LXB 19 15 11.54938 +10 56 44.7585           ~ 2281 0
9 IRAS 19132+1035 Y*O 19 15 38.97768 +10 41 14.4276           ~ 42 0
10 [OF2001] B Rad 19 16.2 +10 27           ~ 1 0
11 SNR G045.7-00.4 SNR 19 16 24.000 +11 09 00.00           ~ 42 0
12 V* V1521 Cyg HXB 20 32 25.78 +40 57 27.9           WN4/5-6/7 1765 2

    Equat.    Gal    SGal    Ecl

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2020.07.04-22:00:16

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