Off-nuclear spectroscopy in NGC 1275

Details Off-nuclear spectroscopy in NGC 1275 Off-nuclear spectroscopy in NGC 1275

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249..560h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, April 1, 1991, p. 560-562. SERC-supported research

Astronomy and Astrophysics

Astronomy

7

Galactic Nuclei, Imaging Techniques, Radio Galaxies, Seyfert Galaxies, Astronomical Spectroscopy, Infrared Imagery, Interstellar Matter, Stellar Color

Scientific paper

Optical and infrared images of the radio galaxy NGC 1275 show a point-like object 7 arcsec north-east of the Seyfert nucleus. This object is still found in the literature described as intrinsic to NGC 1275 and hence extragalactic in origin. An intermediate-dispersion optical spectrum between 3500-4600 A of the 'hotspot' was taken to complement an optical and infrared imaging study of the underlying galaxy in NGC 1275. This object, 7 arcsec north-east of the nucleus, is clearly a foreground star of spectral type F4-F6.

Affiliated with

Also associated with

No associations

Rating

Off-nuclear spectroscopy in NGC 1275 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 Off-nuclear spectroscopy in NGC 1275, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Off-nuclear spectroscopy in NGC 1275 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1793434