Accretion disc spectrum in presence of mass outflow around black holes

dc.contributor.author	Mandal, S.
dc.contributor.author	Kumar, R.
dc.contributor.author	Chattopadhyay, I.
dc.date.accessioned	2015-07-02T11:02:20Z
dc.date.available	2015-07-02T11:02:20Z
dc.date.issued	2013
dc.identifier.uri	http://hdl.handle.net/123456789/1128
dc.description.abstract	We study the effect of mass outflow on the accretion disc spec- trum in presence of heating and cooling processes. Radiation spectrum shows a softening of spectral index in presence of mass outflow. This can explain the state transition of outbursting as well as persistent galactic black hole candidates, in particular when the sources are in hard or intermediate states.	en_US
dc.language.iso	en_US	en_US
dc.publisher	ASI	en_US
dc.relation.ispartofseries	asi8-45
dc.subject	Black hole physics – accretion, accretion discs – radiation mechanisms: general – outflows	en_US
dc.title	Accretion disc spectrum in presence of mass outflow around black holes	en_US
dc.type	Article	en_US