Absorption Dips in the Light Curves of GRO J1655–40 and 4U 1630–47 during Outburst

Using the RXTE PCA, we discovered deep dips in the X-ray light curves of the black hole candidates GRO J1655-40 and 4U 1630-47 during outburst. Similar kind of dips for GRO J1655-40 were found in 90 s measurements of the RXTE ASM during the same outburst. The duration of the dips in both sources is...

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Detalles Bibliográficos
Autores principales: Kuulkers, Erik, Wijnands, Rudy, Belloni, Tomaso, Méndez, Mariano R., Klis, Michiel van der, Paradijs, Jan van
Formato: Articulo
Lenguaje:Inglés
Publicado: 1998
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/123633
Aporte de:
id I19-R120-10915-123633
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
accretion, accretion disks
binaries: close
black hole physics
stars: individual (GRO J1655-40, 4U 1630-47)
X-rays: stars
spellingShingle Ciencias Astronómicas
accretion, accretion disks
binaries: close
black hole physics
stars: individual (GRO J1655-40, 4U 1630-47)
X-rays: stars
Kuulkers, Erik
Wijnands, Rudy
Belloni, Tomaso
Méndez, Mariano R.
Klis, Michiel van der
Paradijs, Jan van
Absorption Dips in the Light Curves of GRO J1655–40 and 4U 1630–47 during Outburst
topic_facet Ciencias Astronómicas
accretion, accretion disks
binaries: close
black hole physics
stars: individual (GRO J1655-40, 4U 1630-47)
X-rays: stars
description Using the RXTE PCA, we discovered deep dips in the X-ray light curves of the black hole candidates GRO J1655-40 and 4U 1630-47 during outburst. Similar kind of dips for GRO J1655-40 were found in 90 s measurements of the RXTE ASM during the same outburst. The duration of the dips in both sources is of the order of minutes. The occurrences of the dips observed with the RXTE PCA and ASM in GRO J1655-40 are consistent with the optically determined orbital period, and were found between photometric orbital phases 0.72 and 0.86. This constitutes the first evidence for orbital variations in X-rays for GRO J1655-40. The PCA data indicate that an absorbing medium is responsible for these dips. The X-ray spectra during the dips can be best described by a heavily absorbed component and an unabsorbed component. In the case of GRO J1655-40 we are able constrain the extent of the absorbing medium and the central X-ray source.
format Articulo
Articulo
author Kuulkers, Erik
Wijnands, Rudy
Belloni, Tomaso
Méndez, Mariano R.
Klis, Michiel van der
Paradijs, Jan van
author_facet Kuulkers, Erik
Wijnands, Rudy
Belloni, Tomaso
Méndez, Mariano R.
Klis, Michiel van der
Paradijs, Jan van
author_sort Kuulkers, Erik
title Absorption Dips in the Light Curves of GRO J1655–40 and 4U 1630–47 during Outburst
title_short Absorption Dips in the Light Curves of GRO J1655–40 and 4U 1630–47 during Outburst
title_full Absorption Dips in the Light Curves of GRO J1655–40 and 4U 1630–47 during Outburst
title_fullStr Absorption Dips in the Light Curves of GRO J1655–40 and 4U 1630–47 during Outburst
title_full_unstemmed Absorption Dips in the Light Curves of GRO J1655–40 and 4U 1630–47 during Outburst
title_sort absorption dips in the light curves of gro j1655–40 and 4u 1630–47 during outburst
publishDate 1998
url http://sedici.unlp.edu.ar/handle/10915/123633
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