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Results on Panoramic Spectroscopy of Mrk 171

Published online by Cambridge University Press:  25 July 2014

S. A. Hakopian ,
S. K. Balayan  and
T. A. Movsessian
S. A. Hakopian
Affiliation:
Byurakan Astrophysical Observatory, (BAO), Byurakan, 0213, Armenia email: susanaha@bao.sci.am
S. K. Balayan
Affiliation:
Byurakan Astrophysical Observatory, (BAO), Byurakan, 0213, Armenia email: susanaha@bao.sci.am
T. A. Movsessian
Affiliation:
Byurakan Astrophysical Observatory, (BAO), Byurakan, 0213, Armenia email: susanaha@bao.sci.am
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Abstract

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Observations of Mrk 171, aimed at conduction of panoramic spectroscopy, were undertaken with the Byurakan 2.6-m telescope using spectrograph “VAGR”. Within the two components of the galaxy, Mrk171W and Mrk171E, there were differentiated eight condensations of starforming activiity, i.e. HII-regions, and no sign of AGN activity was revealed inspite of existing suggestions.

Keywords

Mrk 171NGC 36902D-spectroscopy
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S304: Multiwavelength AGN Surveys and Studies , October 2013 , pp. 411 - 412
Copyright
Copyright © International Astronomical Union 2014 

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