Study of bubble nebula using IUE high resolution spectra

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