Supernova Remnants and Metallicity Trends in NGC 628

Details Supernova Remnants and Metallicity Trends in NGC 628 Supernova Remnants and Metallicity Trends in NGC 628

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aps..osf.p1009m&link_type=abstract

American Physical Society, Ohio Section Fall Meeting, October 19 - 20, 2001 Columbus State Community College; Columbus, Ohio Mee

Physics

Scientific paper

Using several recombination lines of hydrogen, an extinction map of the
nearby face-on spiral galaxy, NGC 628, was generated. Once the
extinction is known, the array of bands used in the continuing study of
supernova remnants and metallicity trends can be corrected and
evaluated.

Affiliated with

Also associated with

No associations

Rating

Supernova Remnants and Metallicity Trends in NGC 628 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 Supernova Remnants and Metallicity Trends in NGC 628, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Supernova Remnants and Metallicity Trends in NGC 628 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1104252