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

Query : 2001A&A...367..613O

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

Full paper

View the references in ADS

Number of rows : 12

N	Identifier	Otype	ICRS (J2000) RA	ICRS (J2000) DEC	Mag U	Mag B	Mag V	Sp type	#ref 1850 - 2023	#notes
1	V* BR Cir	HXB	15 20 40.8532547060	-57 10 00.206639033		21.4	21.4	~	765	1
2	V* V818 Sco	LXB	16 19 55.0692669024	-15 38 25.017666540	11.60	12.40	11.1	Oev	1618	0
3	SS 433	HXB	19 11 49.5647697480	+04 58 57.827127648		16.3	13.0	A7Ib:	2088	4
4	Caswell OH 045.12+00.13	HII	19 13 27.85	+10 53 36.7				~	116	0
5	[OF2001] C	Rad	19 14	+11.5				~	1	0
6	[CKW87] 191147.3+110702	HII	19 14 08.5	+11 12 16				~	27	0
7	IRAS 19124+1106	IR	19 14 45	+11 12.1				~	23	0
8	Granat 1915+105	HXB	19 15 11.55576	+10 56 44.9052				~	2559	0
9	IRAS 19132+1035	Y*O	19 15 38.97768	+10 41 14.4276				~	47	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				~	49	0
12	V* V1521 Cyg	HXB	20 32 25.78	+40 57 27.9				WN4/5-6/7	1903	2

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