Intermediate Galactic Latitude Starforming Region-CG 12

dc.contributor.author	Maheswar, G
dc.contributor.author	Manoj, P
dc.contributor.author	Bhatt, H. C
dc.date.accessioned	2008-07-21T06:23:18Z
dc.date.available	2008-07-21T06:23:18Z
dc.date.issued	2002-09
dc.identifier.citation	BASI, Vol. 30, No. 3, pp. 651 - 652	en
dc.identifier.uri	http://hdl.handle.net/2248/2751
dc.description.abstract	Optical linear polarization measurements of stars seen projected towards CG 12, an intermediate latitude (b = 2P .1) starforming cloud, have been made. The results show that the polarization vectors of the majority of the stars seem to be oriented parallel to the tail of CG 12, implying that the magnetic field in the cloud is parallel to' the tail. Spectroscopic observations of each component of the double star Her 4636 show that only the northern component has Ha in emission.	en
dc.format.extent	74876 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Galactic Latitude	en
dc.subject	Spectroscopic Observations	en
dc.title	Intermediate Galactic Latitude Starforming Region-CG 12	en
dc.type	Article	en