Spectrophotometric investigation of the nucleus of the seyfert galaxy markaryan 308

V. N. Popov; �. E. Khachikyan

doi:10.1007/bf01006262

Spectrophotometric investigation of the nucleus of the seyfert galaxy markaryan 308

Astrophysics ◽

10.1007/bf01006262 ◽

1980 ◽

Vol 16 (1) ◽

pp. 33-36

Author(s):

V. N. Popov ◽

�. E. Khachikyan

Keyword(s):

Seyfert Galaxy ◽

Spectrophotometric Investigation ◽

Galaxy Markaryan

Spectrophotometric investigation of the Seyfert galaxy Markaryan 348

Astrophysics ◽

10.1007/bf01007447 ◽

1979 ◽

Vol 14 (4) ◽

pp. 338-343

Author(s):

V. F. Esipov ◽

V. N. Popov ◽

�. E. Khachikyan

Keyword(s):

Seyfert Galaxy ◽

Spectrophotometric Investigation ◽

Galaxy Markaryan

Velocity field of the Seyfert galaxy Markaryan 744

Astrophysics ◽

10.1007/bf01005582 ◽

1982 ◽

Vol 17 (3) ◽

pp. 221-232 ◽

Cited By ~ 1

Author(s):

V. L. Afanas'ev ◽

A. I. Shapovalova

Keyword(s):

Velocity Field ◽

Seyfert Galaxy ◽

Galaxy Markaryan

Spectrophotometry of the Seyfert galaxy Markaryan 1066

Astrophysics ◽

10.1007/bf01004230 ◽

1982 ◽

Vol 17 (4) ◽

pp. 342-353 ◽

Cited By ~ 1

Author(s):

V. L. Afanas'ev ◽

V. A. Lipovetskii ◽

A. I. Shapovalova

Keyword(s):

Seyfert Galaxy ◽

Galaxy Markaryan

Detailed morphological and spectrophotometric investigation of the galaxy Markaryan 1118

Astrophysics ◽

10.1007/bf01005956 ◽

1989 ◽

Vol 29 (2) ◽

pp. 537-542

Author(s):

A. N. Burenkov ◽

A. R. Petrosyan ◽

A. B. Sarkisyan ◽

�. E. Khachikyan

Keyword(s):

Spectrophotometric Investigation ◽

The Galaxy ◽

Galaxy Markaryan

Spectrophotometry of the Seyfert galaxy Markaryan 744

Astrophysics ◽

10.1007/bf01005373 ◽

1979 ◽

Vol 15 (4) ◽

pp. 376-387

Author(s):

V. L. Afanas'ev ◽

V. A. Lipovetskii ◽

A. I. Shapovalova

Keyword(s):

Seyfert Galaxy ◽

Galaxy Markaryan

Spectrophotometric investigation of the galaxy Markaryan 7

Astrophysics ◽

10.1007/bf01005478 ◽

1990 ◽

Vol 32 (2) ◽

pp. 135-141 ◽

Cited By ~ 3

Author(s):

A. N. Burenkov ◽

�. E. Khachikyan

Keyword(s):

Spectrophotometric Investigation ◽

The Galaxy ◽

Galaxy Markaryan

Investigation of profiles of bright emission lines in the nucleus of the Seyfert galaxy Markaryan 533

Astrophysics ◽

10.1007/bf01005718 ◽

1986 ◽

Vol 24 (3) ◽

pp. 249-253

Author(s):

V. A. Lipovetskii ◽

A. I. Shapovalova ◽

O. A. Dobrodii

Keyword(s):

Seyfert Galaxy ◽

Emission Lines ◽

Bright Emission ◽

Galaxy Markaryan

Hubble Space TelescopeWFPC2 Imaging of the Seyfert Galaxy NGC 3516

The Astrophysical Journal ◽

10.1086/306536 ◽

1998 ◽

Vol 509 (2) ◽

pp. 646-652 ◽

Cited By ~ 16

Author(s):

Pierre Ferruit ◽

Andrew S. Wilson ◽

John S. Mulchaey

Keyword(s):

Seyfert Galaxy

A Radio Study of the Seyfert Galaxy IC 5063: Evidence for Fast Gas Outflow

The Astronomical Journal ◽

10.1086/300236 ◽

1998 ◽

Vol 115 (3) ◽

pp. 915-927 ◽

Cited By ~ 69

Author(s):

R. Morganti ◽

T. Oosterloo ◽

Z. Tsvetanov

Keyword(s):

Seyfert Galaxy

Understanding the origin of radio outflows in Seyfert galaxies using radio polarimetry

Proceedings of the International Astronomical Union ◽

10.1017/s1743921320003014 ◽

2019 ◽

Vol 15 (S356) ◽

pp. 247-251

Author(s):

Biny Sebastian ◽

Preeti Kharb ◽

Christopher P. O’ Dea ◽

Jack F. Gallimore ◽

Stefi A. Baum ◽

...

Keyword(s):

Magnetic Fields ◽

Radio Emission ◽

Active Galactic Nuclei ◽

Galactic Nuclei ◽

Seyfert Galaxy ◽

Seyfert Galaxies ◽

Starburst Galaxies ◽

Galactic Magnetic Fields ◽

5 Ghz

AbstractThe role of starburst winds versus active galactic nuclei (AGN) jets/winds in the formation of the kiloparsec scale radio emission seen in Seyferts is not yet well understood. In order to be able to disentangle the role of various components, we have observed a sample of Seyfert galaxies exhibiting kpc-scale radio emission suggesting outflows, along with a comparison sample of starburst galaxies, with the EVLA B-array in polarimetric mode at 1.4 GHz and 5 GHz. The Seyfert galaxy NGC 2639, shows highly polarized secondary radio lobes, not observed before, which are aligned perpendicular to the known pair of radio lobes. The additional pair of lobes represent an older epoch of emission. A multi-epoch multi-frequency study of the starburst-Seyfert composite galaxy NGC 3079, reveals that the jet together with the starburst superwind and the galactic magnetic fields might be responsible for the well-known 8-shaped radio lobes observed in this galaxy. We find that many of the Seyfert galaxies in our sample show bubble-shaped lobes, which are absent in the starburst galaxies that do not host an AGN.