1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7753
Full metadata record
DC FieldValueLanguage
dc.contributor.authorPavana, M-
dc.contributor.authorAnupama, G. C-
dc.contributor.authorRamya, M. Anche-
dc.contributor.authorKamath, U. S-
dc.contributor.authorSelva Kumar, G-
dc.date.accessioned2021-06-29T06:59:46Z-
dc.date.available2021-06-29T06:59:46Z-
dc.date.issued2020-
dc.identifier.citationProceedings of the International Astronomical Union, Vol. 357, pp. 225 - 229en_US
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/2248/7753-
dc.descriptionRestricted Accessen_US
dc.description.abstractWe present photo-ionization and morpho-kinematic analyses of the ejecta of novae. The sample consists of ten novae belonging to the Fe II, He/N and hybrid classes. The Fe II class of novae in the sample have bipolar cone-like structures, with or without equatorial rings with inclination angle in the range of 40°–60°. The He/N novae have bullet-nose curve along with bipolar cone-like structures and equatorial rings with an inclination angle of ~80°. The hybrid nova in the sample is a bipolar frustum of prolate spheroid along with bipolar cone-like structures and equatorial rings with an inclination angle of 63°.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.relation.urihttps://doi.org/10.1017/S1743921320000216-
dc.rights© International Astronomical Union-
dc.subjectNovaeen_US
dc.subjectCataclysmic variablesen_US
dc.subjectStars : individualen_US
dc.subjectTechniques : spectroscopicen_US
dc.titleGeometry of nova ejectaen_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Geometry of nova ejecta.pdf
  Restricted Access		368.02 kBAdobe PDFView/Open Request a copy
Show simple item record


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