Modelling ionized gas and stellar emissions in starburst components

Details Modelling ionized gas and stellar emissions in starburst components Modelling ionized gas and stellar emissions in starburst components

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002newar..46..203m&link_type=abstract

New Astronomy Reviews, Volume 46, Issue 2-7, p. 203-205.

Astronomy and Astrophysics

Astronomy

Scientific paper

With objectives to model star formation in radio galaxies, we present results of a starburst model, built by coupling the two codes PÉGASE and CLOUDY. Continuum and emission line data are used to derive the properties of a sample of local starbursts. Data are well reproduced with a new relation between the ionization parameter and the metallicity. Colors and Hα equivalent widths indicate that: (i) an underlying stellar population is needed, and (ii) burst ages span the range [0, 6] Myr.

Affiliated with

Also associated with

No associations

Rating

Modelling ionized gas and stellar emissions in starburst components 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 Modelling ionized gas and stellar emissions in starburst components, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modelling ionized gas and stellar emissions in starburst components will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-984810