Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6026
Title: Reddening and dust distribution around V348 SGR
Authors: Kameswara Rao, N
Nandy, K
Keywords: Infrared astronomy;Interstellar extinction;Nebulae;R coronae borealis stars;Black body radiation;Infrared astronomy satellite;Infrared photometry;Sagittarius constellation
Issue Date: 1988
Publisher: Bruxelles : Palais des Académies
Citation: Academie Royale de Belgique, Bulletin De La Classe des Sciences, Vol. 74, No. 11, pp. 376-388
Abstract: Radio and Brackett gamma observations indicate large value of reddening E(B - V) = 1.5 to the nebula surrounding V348 Sgr, where as the star appears to be reddened by only E(B - V) is approximately 0.4. The infrared observations both ground based and with IRAS show that there are two dust components present: the hot dust represented by a 600 K black body longward of 3.5 micron and another cool dust (100 K or less) black body. The hot dust extends to about 6 arcsec radius from the star. The cool dust component surrounds the nebula and probably is responsible for the high extinction in the nebula. A tilted hollow cylinder or a tilted disk with a cavity type structure seems to be needed to account for the lack of reddening toward the star. Similarities of the nebular and dust properties of V348 Sgr and R Cr B indicate that they are approaching the red giant stage for a second time.
URI: http://hdl.handle.net/2248/6026
ISSN: 0001-4141
???metadata.dc.rights???: © Bruxelles : Palais des Académies
???metadata.dc.relation.uri???: http://adsabs.harvard.edu//abs/1988STIA...9049085R
Appears in Collections:IIAP Publications

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