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Diffraction-limited spatial resolution of circumstellar dust shells at 10 micronsA new spatial array instrument has provided diffraction-limited mid-infrared intensity profiles of the type M supergiant stars Alpha Orionis and Alpha Scorpii, both of which are known to exhibit excess 10 micron radiation due to the presence of circumstellar dust shells. In the case of Alpha Ori, there is a marked asymmetry in the dust distribution, with peak intensity of dust emission a distance of 0.9 sec from the star.
Document ID
19840037732
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Bloemhof, E. E.
(Rockwell International Science Center Thousand Oaks, CA, United States)
Townes, C. H.
(Rockwell International Science Center Thousand Oaks, CA, United States)
Vanderwyck, A. H. B.
(Rockwell International Science Center Thousand Oaks, CA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 276
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
84A20519
Funding Number(s)
CONTRACT_GRANT: NSF AST-82-12055
CONTRACT_GRANT: NGL-05-003-272
Distribution Limits
Public
Copyright
Other

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