IRS observations of the dwarf M-star sequence

Details IRS observations of the dwarf M-star sequence IRS observations of the dwarf M-star sequence

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...29h&link_type=abstract

Spitzer Proposal ID #29

Physics

Scientific paper

M-dwarfs are the lowest-mass stars that still undergo a normal main-sequence phase. Studies of these objects are important for two reasons: (1) they are the stellar transition into the brown dwarf classes of objects, and (2) their low photospheric temperatures mean that the chemistry of their atmospheres changes radically as the M-star sequence is traversed. These observations use the IRS to observe a sample of M-dwarfs ranging from M0 to M9.5. The observations generally use the short-low and both high resolution modules.

Affiliated with

Also associated with

No associations

Rating

IRS observations of the dwarf M-star sequence 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 IRS observations of the dwarf M-star sequence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IRS observations of the dwarf M-star sequence will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1823297