Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2725
Title: Fading of light maximum and linear polarization variation in the carbon Mira R Leporis
Authors: Raveendran, A. V
Keywords: Polarization;Stars: Carbon;Circumstellar Matter;Stars: Individual: R Lep;Stars: Variables: Other
Issue Date: Nov-2002
Publisher: Royal Astronomical Society
Citation: Monthly Notice of the Royal Astronomical Society, Vol. 336, No. 3, pp. 992 - 998
Abstract: Polarimetry of R Lep obtained over the years 1991-2002 is presented. During this period the star underwent an episode of fading of the brightness at light maximum, after an interval of about 35 yr. An analysis of the data shows that the percentage linear polarization increased as the fading progressed, attained a maximum of slightly over 3 per cent in the V band close to the epoch of minimum, and remained more or less at the same level during and well after the recovery to normal brightness. The polarization, apparently, originated from the circumstellar envelope above the region where the dust that caused the fading in the star condensed. The physical mechanism that causes the rather large polarization during fadings is perhaps selective extinction by aligned foreground grains produced by the passage of shocks through the circumstellar envelope. The small-amplitude, short-term fluctuations in polarization observed in R Lep, which appear to be superposed on the fading-related large-amplitude variation, are probably pulsation-related and arise from the inner zones of the circumstellar envelope.
URI: http://hdl.handle.net/2248/2725
ISSN: 0035-8711
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/2002MNRAS.336..992R
http://www3.interscience.wiley.com/journal/118945652/abstract
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Raveendran A. V.pdf1.08 MBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.