Chandrahigh-resolution spectra of 4U 1630-47: the disappearance of the wind-Reference-Cited by-同舟云学术

Chandrahigh-resolution spectra of 4U 1630-47: the disappearance of the wind

Published:2018-10-23 Issue:2 Volume:482 Page:2597-2611
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Gatuzz E¹²,Díaz Trigo M¹,Miller-Jones J C A³^ORCID,Migliari S⁴⁵

Affiliation:

1. ESO, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München, Germany

2. Excellence Cluster Universe, Boltzmannstr. 2, D-85748, Garching, Germany

3. International Centre for Radio Astronomy Research, Curtin University, G.PO Box U1987, Perth, WA, 6845, Australia

4. XMM-Newton Science Operations Centre, ESAC/ESA, Camino Bajo del Castillo s/n, Urb. Villafranca del Castillo, 28691 Villanueva de la Cañada, Madrid, Spain

5. Institute of Cosmos Sciences, University of Barcelona, Martí i Franquès 1, E-08028 Barcelona, Spain

Funder

National Radio Astronomy Observatory

National Science Foundation Australian Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/482/2/2597/26559648/sty2850.pdf

Reference80 articles.

1. Three Spectral States of the Disk X-Ray Emission of the Black-Hole Candidate 4U 1630−47

2. The Disk Wind in the Neutron Star Low-mass X-Ray Binary GX 13+1

3. Compton heated winds and coronae above accretion disks. I Dynamics

4. Photoionization instability of the Fe K absorbing plasma in the neutron star transient AX J1745.6-2901

5. Hydromagnetic flows from accretion discs and the production of radio jets

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