Time variation of mid-infrared spectra of M-type Mira variables

Details Time variation of mid-infrared spectra of M-type Mira variables Time variation of mid-infrared spectra of M-type Mira variables

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..257o&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

Mira Variables, Infrared Spectroscopy, Circumstellar Dust

Scientific paper

Time variation of mid-infrared (MIR) spectra of M-type Mira variables has been investigated by ISO/SWS observations of Z Cyg and T Cep. The variation in the Z Cyg spectrum can be accountd for by the variation in the stellar luminosity, if appropriate dust emissivity parameters are adopted. No apparent variation in the spectral shape despite of the intensity variation suggests that emission from high-temperature grains dominates in the MIR spectrum of T Cep.

Affiliated with

Also associated with

No associations

Rating

Time variation of mid-infrared spectra of M-type Mira variables 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 Time variation of mid-infrared spectra of M-type Mira variables, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Time variation of mid-infrared spectra of M-type Mira variables will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-920677