1984NASA conference publicationRequires access

Circumstellar dust disks around young stars.

Martin Cohen, R. Schwartz, P. M. Harvey, B. A. Wilking

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Abstract

Kuiper Airborne Observatory observations of several resolved far-infrared structures that are likely to represent disks formed during the process of the collapse of a cloud to form a star are discussed. An infrared radiation nebula, star HH57, and SVS13 were studied. Forty-seven and 95-micron maps of far infrared radiation are given.

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What this paper is about

Kuiper Airborne Observatory observations of several resolved far-infrared structures that are likely to represent disks formed during the process of the collapse of a cloud to form a star are discussed. An infrared radiation nebula, star HH57, and SVS13 were studied. Forty-seven and 95-micron maps of far infrared radiation are given.

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Available abstract

Kuiper Airborne Observatory observations of several resolved far-infrared structures that are likely to represent disks formed during the process of the collapse of a cloud to form a star are discussed. An infrared radiation nebula, star HH57, and SVS13 were studied. Forty-seven and 95-micron maps of far infrared radiation are given.

Key concepts: Infrared, Circumstellar dust, Physics, Stars, Astronomy, Astrophysics, Nebula, Cosmic dust

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