IRAS04000+5052, a near infrared variable associated with HII region

Details IRAS04000+5052, a near infrared variable associated with HII region IRAS04000+5052, a near infrared variable associated with HII region

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cha%26a..17...61w&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 17, Issue 1, p. 61-64.

Astronomy and Astrophysics

Astrophysics

4

Star, Near Infrared Varible, Hii Region

Scientific paper

Using 2.16m telescope with CCD system at Xinglong station of Beijing Astronomical Observatory, IRAS 04000+5052 has been observed at VRI bands respectively. The R-filter image of the source shows very distinct extension feature. Radiation of the source at R band is much stronger than that at V and I bands. By using the 1.26m infrared telescope, a large variation at near infrared bands was also found. From the IRAS fluxes and LRS spectrum, as well as the morphology of the source, we conclude that it may possibly be a young object in the process forming new stars.

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