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1976•Publications of the Astronomical Society of JapanRequires access

Infrared Photometry of CRL 877 Associated with the Radio Complex in the Monoceros R2 Region

Shuji Sato, Yukiyasu Kobayashi, Kimiaki Kawara, Toshinori Maihara, Haruyuki Okuda

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Abstract

Abstract A position of the bright infrared source CRL 877 is determined as R.A. (1950.0)=6h5m22s±0.s8, Decl. (1950.0) = –6°22′30″ ± 10″. The source is close to a radio complex in the Mon R2 association, involving the compact radio source G213.7—12.6, OH and H2O masers, and molecular clouds. The infrared energy distribution of the source is very similar to that of the BN object in the Orion Nebula with a deep 10-μm depression.

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What this paper is about

Abstract A position of the bright infrared source CRL 877 is determined as R.A. (1950.0)=6h5m22s±0.s8, Decl. (1950.0) = –6°22′30″ ± 10″. The source is close to a radio complex in the Mon R2 association, involving the compact radio source G213.7—12.6, OH and H2O masers, and molecular clouds. The infrared energy distribution of the source is very similar to that of the BN object in the Orion Nebula with a deep 10-μm depression.

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Available abstract

Abstract A position of the bright infrared source CRL 877 is determined as R.A. (1950.0)=6h5m22s±0.s8, Decl. (1950.0) = –6°22′30″ ± 10″. The source is close to a radio complex in the Mon R2 association, involving the compact radio source G213.7—12.6, OH and H2O masers, and molecular clouds. The infrared energy distribution of the source is very similar to that of the BN object in the Orion Nebula with a deep 10-μm depression.

Key concepts: Physics, Photometry (optics), Astrophysics, Astronomy, Infrared, Stars

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