An analysis of the 2.6 - 3.7 micron spectrum of R Dor

Details An analysis of the 2.6 - 3.7 micron spectrum of R Dor An analysis of the 2.6 - 3.7 micron spectrum of R Dor

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..231r&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Stars: Individual (R Dor), Stars: Agb And Post-Agb, Stars: Late-Type, Infrared: Stars

Scientific paper

Here, I present our modelling (Ryde & Eriksson, A&A 2002, 386,
874) of the 2.6 - 3.7 microns spectrum of the red semiregular variable R
Doradus observed with the Short-Wavelength Spectrometer on board the
Infrared Space Obervatory.

Affiliated with

Also associated with

No associations

Rating

An analysis of the 2.6 - 3.7 micron spectrum of R Dor 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 An analysis of the 2.6 - 3.7 micron spectrum of R Dor, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An analysis of the 2.6 - 3.7 micron spectrum of R Dor will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-920627