2011MNRAS.418L..59G


Query : 2011MNRAS.418L..59G

2011MNRAS.418L..59G - Mon. Not. R. Astron. Soc., 418, L59-L63 (2011/November-3)

How the effects of resonant absorption on black hole reflection spectra can mimic high-velocity outflows.

GALLO L.C. and FABIAN A.C.

Abstract (from CDS):

Narrow absorption lines seen in the 2–10 keV spectra of active galaxies and Galactic black holes are normally attributed to iron in high-velocity outflows or inflows. We consider the possibility that such features could arise naturally in the accretion disc. Resonant absorption by highly ionized iron (e.g. Fe XXVI and Fe XXV) in an optically thin plasma that is located above the disc and rotating with it could reproduce narrow features in the reflection component of the spectrum as it emerges from the disc. Depending on the inclination of the disc and the exact geometry of the hot plasma (e.g. whether it blanket the disc or a ring), apparently narrow absorption features could be detected between 4 and 10 keV. Such an explanation requires no high-velocity outflow/inflow and is consistent with a reflection-based interpretation for accreting black holes systems.

Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS

Journal keyword(s): accretion, accretion discs - black hole physics - line: formation - line: identification - relativistic processes - galaxies: active

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 : 2011MNRAS.418L..59G

Basic data :
V* V1033 Sco -- High Mass X-ray Binary
Other object types:
otypes_help
X (2008ApJ,PBC,...), * (UCAC4,ChOPS,...), LXB (2013ApJS), V* (V*,AAVSO), gam (GRO,INTREF), HXB (2012ApJ), No* (NOVA), NIR (2MASS)
ICRS coord. (ep=J2000) :
16 54 00.1423963019 -39 50 44.761701340 (Optical) [ 0.0438 0.0276 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
16 50 33.1097810893 -39 45 52.417537282 [ 0.0438 0.0276 90 ]
Gal coord. (ep=J2000) :
344.9819404282615 +02.4559750537325 [ 0.0438 0.0276 90 ]
Proper motions mas/yr :
-4.329 -7.461 [0.062 0.047 90] A 2020yCat.1350....0G
Parallaxes (mas):
0.2902 [0.0481] A 2020yCat.1350....0G
Spectral type:
F3-6IV D 2008ApJ...685..463K
Fluxes (5) :
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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Identifiers (17) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

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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Collections of Measurements Description of Measurements

Distance : 1    Plx : 1    PM : 1    SpT : 1   

   

Observing logs
XMM : 7   

   


External archives :

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

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

Link by name to the catalogue in VizieR :

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

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