Spectroscopy of the Extended Emission Line Region in NGC 4388

Details Spectroscopy of the Extended Emission Line Region in NGC 4388 Spectroscopy of the Extended Emission Line Region in NGC 4388

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..123t&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 123-126 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present preliminary results of long-slit spectroscopic observations of the extended emission line region (hereafter, EELR) in NGC 4388. We detect broad emission lines in the line complexes Hα+[NII] and [SII] which can be modelled by the superposition of several narrow components. Multicomponent line profiles appear at positions very close to the ionization cone axis. There is also some correspondence with the radio emission, which suggests that there is interaction between the radio jets and the ionized gas. We do not confirm the claim of a broad Hα component (FWZI=4000 km/s) by Shields and Filippenko (1996).

Affiliated with

Also associated with

No associations

Rating

Spectroscopy of the Extended Emission Line Region in NGC 4388 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 Spectroscopy of the Extended Emission Line Region in NGC 4388, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopy of the Extended Emission Line Region in NGC 4388 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1330983