Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3873
Title: CN 1-1 - A peculiar compact planetary nebula
Authors: Bhatt, H. C
Mallik, D. C. V
Keywords: Binary stars;Emission spectra;Infrared spectra;Line spectra;Planetary nebulae;Protoplanets;Computational astrophysics;F stars;Far infrared radiation;Infrared astronomy satellite;Stellar evolution;Stellar luminosity;Stellar temperature
Issue Date: Nov-1986
Publisher: The European Southern Observatory
Citation: Astronomy and Astrophysics , Vol. 168, No. 1 - 2, pp. 248 - 252
Abstract: Cn 1-1 is an emission-line object that shows strong emission lines characteristic of high density planetary nebulae superposed on the stellar spectrum of an F5 III-IV star. The authors estimate the absolute luminosity of the hot star of Cn 1-1 to be L* ≅ 63 L_sun;. A new estimate of the effective temperature of the star is also made based on the IRAS and IUE data. The position of the star on the HR diagram is discrepant with the young age of the nebula as deduced from the high nebular density. In addition to the cool dust at ≅215K there is a second distinct hot dust component at ≅850K that is probably heated by the radiation from the F type star in its neighbourhood, the star being embedded in the cool nebular dust. Cn 1-1 may be a Type I protoplanetary nebula with a massive nucleus (M ⪆ 1.2 M_sun;) evolving in a binary system.
URI: http://hdl.handle.net/2248/3873
ISSN: 0004-6361
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1986A%26A...168..248B
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
A peculiar compact planetary nebula847.1 kBAdobe PDFView/Open


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