Velocity field structure in the Orion Nebula

dc.contributor.author	Seema, P
dc.contributor.author	Banerjee, D. P. K
dc.contributor.author	Anandarao, B. G
dc.date.accessioned	2007-05-09T08:32:45Z
dc.date.available	2007-05-09T08:32:45Z
dc.date.issued	1993
dc.identifier.citation	BASI, Vol. 21, pp. 569-573	en
dc.identifier.uri	http://hdl.handle.net/2248/1556
dc.description.abstract	High quality interferograms have been obtained on the H II region in the Orion Nebula in the emission line of (OIII) 5007 A using the high resolution imaging Fabry-Perot spectrometer. Velocity profiles were obtained for about 2000 spatial positions. Two velocity components, a narrow one with full width at half maximum (FWHM) of around 20 +/- 3 km/sec and a broad one with FWHM of around 50 +/- 3 km/sec are predominantly present in the profiles across the nebula	en
dc.format.extent	364261 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Orion nebula	en
dc.subject	Velocity structure	en
dc.title	Velocity field structure in the Orion Nebula	en
dc.type	Article	en