The star formation rate in nearby spiral galaxies

Details The star formation rate in nearby spiral galaxies The star formation rate in nearby spiral galaxies

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..395b&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Star Formation Rate (SFR) (and its spatial variation within a
galaxy) is a very important ingredient of galactic evolution and aspect.
In nearby disk galaxies, fortunately, both theories and observations
concerning the SFR do exist. We present recent results obtained by
comparing the former to the latter.

Affiliated with

Also associated with

No associations

Rating

The star formation rate in nearby spiral galaxies 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 star formation rate in nearby spiral galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The star formation rate in nearby spiral galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1201138