Gas and stars in compact (young) radio sources

Details Gas and stars in compact (young) radio sources Gas and stars in compact (young) radio sources

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009an....330..233m&link_type=abstract

Astronomische Nachrichten, Vol.330, Issue 2, p.233

Astronomy and Astrophysics

Astronomy

7

Galaxies: Active, Galaxies: Evolution, Galaxies: Ism

Scientific paper

Gas can be used to trace the formation and evolution of galaxies as well as the impact that the nuclear activity has on the surrounding medium. For nearby compact radio sources, we have used observations of neutral hydrogen - that we detected in emission distributed over very large scales - combined with the study of the stellar population and deep optical images to investigate the history of the formation of their host galaxy and the triggering of the activity. For more distant and more powerful compact radio sources, we have used optical spectra and H I - in absorption - to investigate the presence of fast outflows that support the idea that compact radio sources are young radio loud AGN observed during the early stages of their evolution and currently shredding their natal cocoons through extreme circumnuclear outflows. We will review the most recent results obtained from these projects.

Affiliated with

Also associated with

No associations

Rating

Gas and stars in compact (young) radio sources 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 Gas and stars in compact (young) radio sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gas and stars in compact (young) radio sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-836374