Computer Science – Databases
Scientific paper
Mar 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002stin...0239428s&link_type=abstract
Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States
Computer Science
Databases
Infrared Spectroscopy, Molecular Clouds, Star Formation, Infrared Radiation, Spectrometers, Stellar Mass, Galaxies
Scientific paper
This report details work done in a project involving spectroscopic studies, including data analysis and modeling, of star-formation regions using an ensemble of archival space-based data including some from the Infrared Space Observatory's Long Wavelength Spectrometer and Short Wavelength Spectrometer, and other spectroscopic databases. We will include four kinds of regions: (1) disks around more evolved objects; (2) young, low or high mass pre-main sequence stars in star-formation regions; (3) star formation in external, bright IR (infrared) galaxies; and (4) the galactic center. During this period, work proceeded fully on track and on time. Details on workshops and conferences attended and research results are presented. A preprint article entitled 'The Far Infrared Lines of OH as Molecular Cloud Diagnostics' is included as an appendix.
No associations
LandOfFree
Infrared Spectroscopy of Star Formation in Galactic and Extragalactic Regions 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 Infrared Spectroscopy of Star Formation in Galactic and Extragalactic Regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infrared Spectroscopy of Star Formation in Galactic and Extragalactic Regions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1498670