Study of bubble nebula using IUE high resolution spectra

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4724

Full metadata record

DC Field	Value	Language
dc.contributor.author	Anand, M. Y	-
dc.contributor.author	Kagali, B. A	-
dc.contributor.author	Murthy, J	-
dc.date.accessioned	2009-08-06T10:30:54Z	-
dc.date.available	2009-08-06T10:30:54Z	-
dc.date.issued	2009-06	-
dc.identifier.citation	Bulletin of the Astronomical Society of India, Vol. 37, No. 1 & 2, pp. 1 - 10	en
dc.identifier.issn	0304-9523	-
dc.identifier.uri	http://hdl.handle.net/2248/4724	-
dc.description.abstract	In this paper, we have analyzed IUE high resolution spectra of the central star (BD+602522) of the Bubble nebula. We discuss velocities of the different regions along the line of sight to the bubble. We find that the Bubble nebula is younger (by a factor of 100) than the exciting star suggesting that either the bubble is expanding into an inhomogeneous interstellar medium or that the mechanics of the stellar wind are not fully understood.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.rights	© Astronomical Society of India	en
dc.subject	Bubbles	en
dc.subject	Data Analysis	en
dc.subject	Line Identification	en
dc.title	Study of bubble nebula using IUE high resolution spectra	en
dc.type	Article	en
Appears in Collections:	BASI Publications IIAP Publications

Files in This Item:

File	Description	Size	Format
Study of Bubble nebula using IUE high resolution spectra		229.89 kB	Adobe PDF	View/Open

DSpace JSPUI