IIA Institutional Repository

Hard X-ray flux variations in AGN from NuSTAR

Show simple item record

dc.contributor.author Priyanka Rani
dc.contributor.author Stalin, C. S
dc.date.accessioned 2020-11-27T01:24:52Z
dc.date.available 2020-11-27T01:24:52Z
dc.date.issued 2015-04
dc.identifier.citation ASI Conference Series, Vol. 12, pp. 135-136 en_US
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7472
dc.description Open Access © Astronomical Society of India http://www.astron-soc.in/bulletin/asics_vol012/pdfs/priyanka.pdf en_US
dc.description.abstract We present here our results on the hour like time scale Xray flux variations in a sample of active galactic nuclei using data from the Nuclear Spectroscopic Telescope Array (NuSTAR). We find that in the 3−79 keV band, BL Lacs are more variable than flat spectrum radio quasars and Seyfert galaxies. Among Seyferts, Seyfert 2s are more variable than Seyfert 1s. Also, radio-loud quasars are more variable in the hard (10−79 keV) band than the soft (3−10 keV) band while, Seyfert galaxies tend to show more variations in the soft band relative to the hard band. en_US
dc.language.iso en en_US
dc.publisher Astronomical Society of India en_US
dc.subject Galaxies: active en_US
dc.subject galaxies:Seyfert en_US
dc.subject - BL Lacertae objects:general en_US
dc.title Hard X-ray flux variations in AGN from NuSTAR en_US
dc.type Article en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account