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The continuing saga of Sakurai's object (V4334 Sgr): dust production and helium line emission
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
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2000 (English)In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, Vol. 315, no 3, 595-599 p.Article in journal (Refereed) Published
Abstract [en]

We report further UKIRT spectroscopic observations of Sakurai's object (V4334 Sgr) made in 1999 April/May in the 1-4.75 mu m range, and find that the emission is dominated by amorphous carbon at T-d similar to 600 K. The estimated maximum grain size is 0.

Place, publisher, year, edition, pages
BLACKWELL SCIENCE LTD , 2000. Vol. 315, no 3, 595-599 p.
Keyword [en]
stars : AGB and post-AGB; circumstellar matter; stars : individual : Sakurai's; object; stars : individual : V4334 Sgr; infrared : stars
Identifiers
URN: urn:nbn:se:uu:diva-36668OAI: oai:DiVA.org:uu-36668DiVA: diva2:64567
Note
Addresses: Tyne VH, Univ Keele, Dept Phys, Keele ST5 5BG, Staffs, England. Univ Keele, Dept Phys, Keele ST5 5BG, Staffs, England. Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead CH41 1LD, Merseyside, England. Gemini Observ, Hilo, HI 96720 USA.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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