Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005assl..329p..23h&link_type=abstract
Starbursts: From 30 Doradus to Lyman Break Galaxies, Held in Cambridge, UK, 6-10 September 2004. Edited by R. de Grijs and R.M.
Astronomy and Astrophysics
Astrophysics
1
Scientific paper
The star-formation rate (SFR) of spiral galaxies seems to follow a relationship with their morphological type: the later the type of the galaxy, the larger the SFR becomes. Here, we will present SFRs, derived from Hα images, of a sample of late-type, inactive, non-peculiar spirals. The common property is that all these galaxies have radii smaller than 5 kpc. Two important (and shocking!) results come out: the SFRs of dwarf late-type spirals are lower than expected. Moreover, the number of H II regions as well as the SFRs is larger for barred dwarf galaxies. Therefore, the question arises: is size a key parameter in Star-Formation Rates of spiral galaxies?
No associations
LandOfFree
Does size matter (in the SFRs)? 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 Does size matter (in the SFRs)?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Does size matter (in the SFRs)? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1701737