2006ApJ...652L.117N

Query : 2006ApJ...652L.117N

2006ApJ...652L.117N - Astrophys. J., 652, L117-L120 (2006/December-1)

A thermal wind model for the X-ray outflow in GRO J1655-40.

NETZER H.

Abstract (from CDS):

Recent Chandra observations of an outflowing gas in GRO J1655-40 resulted in a suggestion by Miller et al. that the wind in this system must be powered by a magnetic process that can also drive accretion through the disk around the black hole. The alternative explanations, of radiation pressure or thermally driven flows, were considered unsatisfactory because of the highly ionized level of the gas and because of the derived small distance from the black hole, well inside the minimum distance required for an efficient X-ray-heated wind. The present Letter shows that there is a simple photoionized wind solution for this system where the gas is much farther out than assumed by Miller et al., at r/r_g=10^4.7-10^5.7. The expected wind velocity, as well as the computed equivalent widths of more than 50 absorption lines in this single-component one-dimensional model, are all in good agreement with the Chandra observations.

Abstract Copyright: ∼

Journal keyword(s): Accretion, Accretion Disks - Stars: Binaries: Spectroscopic - Black Hole Physics - Stars: Individual: Alphanumeric: GRO J1655-40 - X-Rays: Stars

Simbad objects: 1

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Number of rows : 1

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	V* V1033 Sco	HXB	16 54 00.1423963019	-39 50 44.761701340				16.14		F3-6IV	1980	0

Query : 2006ApJ...652L.117N

Basic data :

V* V1033 Sco -- High Mass X-ray Binary

X (2008ApJ,PBC,...), * (UCAC4,ChOPS,...), LXB (2013ApJS), V* (V*,AAVSO), gam (GRO,INTREF), HXB (2012ApJ), No* (NOVA), NIR (2MASS)

16 54 00.1423963019 -39 50 44.761701340 (Optical) [ 0.0438 0.0276 90 ] A 2020yCat.1350....0G

16 50 33.1097810893 -39 45 52.417537282 [ 0.0438 0.0276 90 ]

344.9819404282615 +02.4559750537325 [ 0.0438 0.0276 90 ]

-4.329 -7.461 [0.062 0.047 90] A 2020yCat.1350....0G

0.2902 [0.0481] A 2020yCat.1350....0G

F3-6IV D 2008ApJ...685..463K

R 16.14 [0.01] C 2008ApJ...685..463K

G 16.226719 [0.005626] C 2022yCat.1355....0G

J 13.516 [0.029] C 2003yCat.2246....0C

H 12.997 [0.044] C 2003yCat.2246....0C

K 12.744 [0.034] C 2003yCat.2246....0C

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`UCAC4 251-103937`	`INTREF 727`	`SWIFT J1654.0-3950`	`AAVSO 1647-39`
`ChOPS J165400.14-395045.1`	`2MASS J16540014-3950447`	`TIC 339434742`	`Gaia DR3 5969790961312131456`
`GRO J1655-40`	`NOVA Sco 1994`	*`V V1033 Sco`**
`GRO J1655-44`	`PBC J1653.9-3950`	`2XMM J165400.1-395044`
`GRO J1655-41`	`SWIFT J1653.8-3952`	`[KRL2007b] 208`

References (1980 between 1850 and 2026) (Total 1980)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).

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Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : V* V1033 Sco

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UCAC4 251-103937 2MASS J16540014-3950447 V* V1033 Sco Gaia DR3 5969790961312131456

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