The Infrared Development of V705 Cassiopeiae

Details The Infrared Development of V705 Cassiopeiae The Infrared Development of V705 Cassiopeiae

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...494..783m&link_type=abstract

Astrophysical Journal v.494, p.783

Astronomy and Astrophysics

Astronomy

17

Stars: Circumstellar Matter, Ism: Dust, Extinction, Infrared: Stars, Stars: Novae, Cataclysmic Variables, Stars: Individual Constellation Name: V705 Cassiopeiae

Scientific paper

We report 1.2-18.5 mu m spectrophotometric measurements of the CO nova V705 Cassiopeiae (Nova Cas 1993). Observations were made over a 2.5 yr period between 7.1 and 929.4 days past outburst. This time frame was marked by all major phases of nova evolution. An optically thick, carbon dust shell formed by day 70.9. Later evolutionary stages of the dust shell are modeled using a combination of emission from carbon, silicate, and hydrocarbon grains. Using this model, we estimate carbon, silicate, and gas abundances in addition to several other calculable physical parameters.

Affiliated with

Also associated with

No associations

Rating

The Infrared Development of V705 Cassiopeiae 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 The Infrared Development of V705 Cassiopeiae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Infrared Development of V705 Cassiopeiae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1223323