Recent observations concerning the morphology of the galaxy NGC 2997 and its hot spots

Details Recent observations concerning the morphology of the galaxy NGC 2997 and its hot spots Recent observations concerning the morphology of the galaxy NGC 2997 and its hot spots

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pasp...92...38m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 92, Feb.-Mar. 1980, p. 38-42.

Astronomy and Astrophysics

Astronomy

6

Galactic Structure, H Alpha Line, Spiral Galaxies, Stellar Luminosity, Astronomical Catalogs, Galactic Nuclei, H Ii Regions, Hydrogen Ions, Telescopes

Scientific paper

Recent observations with the 3.60-m ESO telescope show that the hot spots surrounding the nucleus of NGC 2997 appear as a ring in H-alpha light. The galaxy is found to be inclined 45 deg with respect to the plane of the sky; this can be interpreted as the elliptical H II tore in the plane of NGC 2997 of strong eccentricity, or an H II bubble. The hot spots have a brightness similar to the brightest stellar associations and H II regions of the spiral arms, and about ten times the brightness of the conventional chains of H II regions defining the arms.

Affiliated with

Also associated with

No associations

Rating

Recent observations concerning the morphology of the galaxy NGC 2997 and its hot spots 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 Recent observations concerning the morphology of the galaxy NGC 2997 and its hot spots, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Recent observations concerning the morphology of the galaxy NGC 2997 and its hot spots will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1622242