ARIES-Institutional Digital Repository

Spectrophotometry of comet Bradfield (1980t) during post-perihelion period

Show simple item record

dc.contributor.author Goraya, P. S.
dc.contributor.author Sinha, B. K.
dc.contributor.author Chaubey, U. S.
dc.contributor.author Sanwal, B. B.
dc.date.accessioned 2010-03-25T08:50:38Z
dc.date.available 2010-03-25T08:50:38Z
dc.date.issued 1982
dc.identifier.uri http://hdl.handle.net/123456789/642
dc.description.abstract Spectrum scans of the head of comet Bradfield (1980t) covering the wavelength range λ λ365-640 nm were made on two nights when the heliocentric distance of the comet varied from 0.55 to 0.58 AU. The emission features of the CN band at λ388 nm and Swan band sequence of C₂ at λ474 nm, λ516nm, and λ563 nm are identified and absolute fluxes in these bands as well as in the continuum are derived. The continuum energy distribution curves of the comet have been compared with those of the Sun and the star β Crv (G5 III). An estimate of the number of C₂ and CN molecules in the head of the comet has been made through the measured intensities of their respective bands lying in this region. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries emp26-3
dc.subject Comet Bradfield (1980t), Spectrophotometry en_US
dc.title Spectrophotometry of comet Bradfield (1980t) during post-perihelion period en_US
dc.type Article en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search ARIES-IDR


Advanced Search

Browse

My Account

Context