NV Aurigae - an optically thick Mira star

Details NV Aurigae - an optically thick Mira star NV Aurigae - an optically thick Mira star

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cha%26a..16..293w&link_type=abstract

Chinese Astronomy and Astrophysics (ISSN 0275-1062) Translation., vol. 16, no. 3, p. 293-300.

Astronomy and Astrophysics

Astrophysics

Asymptotic Giant Branch Stars, Auriga Constellation, Cosmic Dust, Infrared Photometry, Mira Variables, Optical Thickness, Astronomical Observatories, Charge Coupled Devices, Infrared Telescopes, Schmidt Telescopes

Scientific paper

The physical parameters of the NV Aur dust shell and central star were derived using optical and NIR data obtained by the 1.26-m IR telescope and the 60/90 cm CCD-equipped Schmidt telescope at the Xinglong Station, Beijing Astronomical Observatory, together with IRAS data. The results of the morphological analysis of the IRAS-LRS spectrum indicate that NV Aur is a Mira star that has just entered the optically thick stage. The results on NV Aur are used to derive a blackbody spectrum model.

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