Probing the physics of Seyfert galaxies using their emission-line regions

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7332

Title:	Probing the physics of Seyfert galaxies using their emission-line regions
Authors:	Shastri, P Dopita, M Scharwachter, J Kewley, L Davies, R Sutherland, R Kharb, P Banfield, J Jose, J Ramya, S Srivastava, S Bhatt, H. C Hampton, E Jin, J Basurah, H Fischer, S Gupta, M Panda, S Sundar, M. N Radhakrishnan, V
Keywords:	Galaxies: active
Issue Date:	Dec-2015
Publisher:	AIP Publishing
Citation:	AIP Conference Proceedings, Vol.1697, pp. 110002-3
Abstract:	Active galaxies have powerhouses of radiation in their nuclear regions that are driven by accreting super-massive black holes. The accretion system also generates outflows of ionized gas and synchrotron-emitting bipolar jets of plasma, which could have a significant impact on the host galaxy. We have initiated an investigation into the physics of nearby active galaxies by studying the morphology, kinematics, excitation abundance structure, and radio structure of about 120 nearby targets. We present a few early results from this investigation.
Description:	Restricted Access © AIP Publishing http://dx.doi.org/10.1063/1.4937705
URI:	http://prints.iiap.res.in/handle/2248/7332
ISSN:	0094-243X
Appears in Collections:	IIAP Publications

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