Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.313..297w&link_type=abstract
Astrophysics and Space Science, Volume 313, Issue 1-3, pp. 297-302
Astronomy and Astrophysics
Astrophysics
Galaxies: Infrared, Galaxies: Ism, Galaxies: Individual (Mrk231, Mrk273, Ugc5101, Iras10565+2448)
Scientific paper
Luminous and Ultraluminous infrared galaxies (ULIRGs) contain the most intense regions of star formation in the local universe. Because molecular gas is the fuel for current and future star formation, the physical properties and distribution of the warm, dense molecular gas are key components for understanding the processes and timescales controlling star formation in these merger and merger remnant galaxies. We present new results from a legacy project on the Submillimeter Array which is producing high resolution images of a representative sample of galaxies with log L FIR >11.4 and D<200 Mpc.
Armus Lee
Baker Andrew Jordan
Cox Theodore J.
Ho Pak Tung
Iono Daisuke
No associations
LandOfFree
Luminous infrared galaxies with the submillimeter array: probing the extremes of star formation 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 Luminous infrared galaxies with the submillimeter array: probing the extremes of star formation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Luminous infrared galaxies with the submillimeter array: probing the extremes of star formation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1593160