How to measure the gas mass: predictions for JCMT, APEX, Herschel and SOFIA

Details How to measure the gas mass: predictions for JCMT, APEX, Herschel and SOFIA How to measure the gas mass: predictions for JCMT, APEX, Herschel and SOFIA

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005nrdd.conf...14k&link_type=abstract

Proceedings of the Miniworkshop on Nearby Resolved Debris Disks. October 19-20, 2005. Space Telescope Science Institute, Baltimo

Computer Science

Scientific paper

Two fundamental questions in the context of these debris disks are: 1) How much gas is left in the disks? 2) What is the nature of the gas in the disk: primordial gas or outgassing comets? We present here a parameter study using disk models that span a range of 4 orders of magnitude in disk mass (1.5 10^{-4} - 1.5 10^{-8} M_Sun). Integrated line emission for various tracers - CO, O, C+ - is computed as a function of disk mass for present and upcoming observing facilities such as ALMA, SOFIA and Herschel.

Affiliated with

Also associated with

No associations

Rating

How to measure the gas mass: predictions for JCMT, APEX, Herschel and SOFIA 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 How to measure the gas mass: predictions for JCMT, APEX, Herschel and SOFIA, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and How to measure the gas mass: predictions for JCMT, APEX, Herschel and SOFIA will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1382734