OH MM/ULIRGs at High Redshifts: What Can They Tell Us ?

Details OH MM/ULIRGs at High Redshifts: What Can They Tell Us ? OH MM/ULIRGs at High Redshifts: What Can They Tell Us ?

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..407...73b&link_type=abstract

The Low-Frequency Radio Universe ASP Conference Series, Vol. 407, proceedings of the conference held 8-12 December 2008, at Nati

Astronomy and Astrophysics

Astrophysics

Scientific paper

OH MegaMaser activity as observed in the nearby Universe provides opportunities to study the population of active galaxies at significantly higher redshifts. The understanding of the OH emission phenomenology in nearby ULIRGs may be used to add to the diagnostics of the properties of the SMG population. We discuss the interpretation of observational data of nearby galaxies with a nuclear ISM that supports OH MM emission and the predictions that can be made about the detection of OH MM at higher redshifts.

Affiliated with

Also associated with

No associations

Rating

OH MM/ULIRGs at High Redshifts: What Can They Tell Us ? 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 OH MM/ULIRGs at High Redshifts: What Can They Tell Us ?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and OH MM/ULIRGs at High Redshifts: What Can They Tell Us ? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-834139