Magnetic fields in cometary globules - II. CG 30-31 complex

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3282

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DC Field	Value	Language
dc.contributor.author	Bhatt, H. C	-
dc.date.accessioned	2008-09-01T09:17:25Z	-
dc.date.available	2008-09-01T09:17:25Z	-
dc.date.issued	1999-09	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, Vol. 308, No. 1, pp. 40 - 44	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2248/3282	-
dc.description.abstract	Optical linear polarization measurements of stars in the region of the cometary globules CG 30-31 in Vela-Puppis are presented. A polarization map representing the geometry of the magnetic field in the cometary globule complex is produced. The magnetic field is found to be nearly perpendicular to the cometary tails. This is unlike the case of the cometary globule CG 22 in which the field had earlier been found to be aligned with the tail. The observed field direction is more or less parallel to the bipolar molecular outflow from the young stellar object IRS 4 embedded in the head of CG 30.	en
dc.language.iso	en	en
dc.publisher	The Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1999MNRAS.308...40B	en
dc.subject	Magnetic fields	en
dc.subject	Cometary globules - II	en
dc.title	Magnetic fields in cometary globules - II. CG 30-31 complex	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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