The search for binary black holes in Seyferts with double peaked emission lines

dc.contributor.author	Kharb, P
dc.contributor.author	Mousumi Das
dc.contributor.author	Subramanian, S
dc.contributor.author	Paragi, Z
dc.date.accessioned	2020-11-27T01:25:23Z
dc.date.available	2020-11-27T01:25:23Z
dc.date.issued	2015-04
dc.identifier.citation	ASI Conference Series, Vol. 12, pp. 65-68	en_US
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/7476
dc.description	Open Access © Astronomical Society of India http://www.astron-soc.in/bulletin/asics_vol012/pdfs/preeti.pdf	en_US
dc.description.abstract	We discuss results from very long baseline interferometry (VLBI) observations of two Seyfert galaxies with double peaked emission lines in their SDSS optical spectra. Such AGN are potential candidates for the presence of binary black holes, which can be resolved on parsec-scales with VLBI. Our observations do not detect twin radio cores but rather nuclear outflows in these Seyferts. These outflows could be interacting with the emission line clouds producing the double peaks in the emission lines	en_US
dc.language.iso	en	en_US
dc.publisher	Astronomical Society of India	en_US
dc.subject	galaxies: nuclei	en_US
dc.subject	galaxies: Seyfert	en_US
dc.subject	radio continuum: galaxies	en_US
dc.title	The search for binary black holes in Seyferts with double peaked emission lines	en_US
dc.type	Article	en_US