Photoionization and Shock Modelling of the H II Region Abundance Sequence and of Luminous Infrared Galaxies

Details Photoionization and Shock Modelling of the H II Region Abundance Sequence and of Luminous Infrared Galaxies Photoionization and Shock Modelling of the H II Region Abundance Sequence and of Luminous Infrared Galaxies

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000rmxac...9..163k&link_type=abstract

"Astrophysical Plasmas: Codes, Models, and Observations, Proceedings of the conference held in Mexico City, October 25-29, 1999,

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

We recalibrate the abundance sequence for extragalactic H II regions and
compare photoionization and shock models for a luminous sub-sample of
southern starburst galaxies. We find H II regions are young. Luminous IR
galaxies are excited by continuous star formation and/or AGN and have
higher than solar metallicity.

Affiliated with

Also associated with

No associations

Rating

Photoionization and Shock Modelling of the H II Region Abundance Sequence and of Luminous Infrared 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 Photoionization and Shock Modelling of the H II Region Abundance Sequence and of Luminous Infrared Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photoionization and Shock Modelling of the H II Region Abundance Sequence and of Luminous Infrared Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1347170