The Redshift and Classification of IGR J20187+4041: A Low- Luminosity Seyfert Galaxy Behind the Galactic Plane in Cygnus

Details The Redshift and Classification of IGR J20187+4041: A Low- Luminosity Seyfert Galaxy Behind the Galactic Plane in Cygnus The Redshift and Classification of IGR J20187+4041: A Low- Luminosity Seyfert Galaxy Behind the Galactic Plane in Cygnus

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1623....1g&link_type=abstract

The Astronomer's Telegram, #1623

Astronomy and Astrophysics

Astronomy

2

Radio, Optical, X-Ray, Gamma Ray, Agn

Scientific paper

A spectrum of 2MASX J20183871+4041003, the galaxy counterpart of IGR J20187+4041, was obtained on 2008 May 5 UT using DEIMOS on the Keck II telescope, covering the wavelength range 6656-9275 Å at 1.2" resolution. Seeing was ~0.5", and the nucleus was isolated using a 0.7" wide slit. Narrow (FWHM ~300 km/s) emission lines of Hα, [N II] 6583, [S II] 6716,6730, and [S III] 9068 are detected at z = 0.0144.

Affiliated with

Also associated with

No associations

Rating

The Redshift and Classification of IGR J20187+4041: A Low- Luminosity Seyfert Galaxy Behind the Galactic Plane in Cygnus does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Redshift and Classification of IGR J20187+4041: A Low- Luminosity Seyfert Galaxy Behind the Galactic Plane in Cygnus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Redshift and Classification of IGR J20187+4041: A Low- Luminosity Seyfert Galaxy Behind the Galactic Plane in Cygnus will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1360447