New pulsating variables discovered from the Naini Tal-Cape survey

dc.contributor.author	Seetha, S
dc.contributor.author	Ashoka, B. N
dc.contributor.author	Joshi, S
dc.contributor.author	Girish, V
dc.contributor.author	Sagar, R
dc.contributor.author	Chaubey, U. S
dc.contributor.author	Gupta, S. K
dc.date.accessioned	2008-07-17T12:08:53Z
dc.date.available	2008-07-17T12:08:53Z
dc.date.issued	2002-09
dc.identifier.citation	BASI, Vol. 30, No. 3, pp. 623 - 629	en
dc.identifier.uri	http://hdl.handle.net/2248/2732
dc.description.abstract	The Naini Tal-Cape survey has been initiated to search for pulsations in chemically peculiar A and F type stars. Many of the magnetic A peculiar type stars exhibit rapid oscillations with periods ranging from 4-16 minutes. These stars are termed as rapidly oscillating Ap stars (roAp) stars. The oscillations are attributed to low order, high overtone p modes. In addition to the Ap stars, this region of the HR diagram also encompasses the non-magnetic 'Am' or metallic lined stars. Some of these Am stars exhibit low overtone 6 Scuti type pulsations. The scientific motivation for a study of these oscillations is discussed along with the results on the variables discovered from the survey.	en
dc.format.extent	223841 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	roAP-CP-pulsations-stars	en
dc.subject	HD 12098 13038-HD 13079-HD 98851	en
dc.title	New pulsating variables discovered from the Naini Tal-Cape survey	en
dc.type	Article	en