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A possible interpretation of the optical spectrum for BL Lac-type objects

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dc.contributor.author Nazarova L.
dc.contributor.author Zentsova A.
dc.date.accessioned 2018-09-14T20:04:50Z
dc.date.available 2018-09-14T20:04:50Z
dc.date.issued 1984
dc.identifier.issn 0004-640X
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/132102
dc.description.abstract On the basis of Sobolev's method, the population of 30 levels of hydrogen atom is determined allowing for the radiative and collision processes of the heating and ionization of the medium with velocity gradient grad v=10-9-10-11s-1, electron temperature Te=104 K-2×104 K and electron density Ne=1010 cm-3-1011 cm-3. The central source radiation is characterized by a power spectrum with spectral indices varying from 0 to 2. A region of possible physical conditions is found where the thermal diffuse radiation of the envelope exceeds the emission in the Balmer Hβ line. © 1984 D. Reidel Publishing Company.
dc.relation.ispartofseries Astrophysics and Space Science
dc.title A possible interpretation of the optical spectrum for BL Lac-type objects
dc.type Article
dc.relation.ispartofseries-issue 1-2
dc.relation.ispartofseries-volume 100
dc.collection Публикации сотрудников КФУ
dc.relation.startpage 301
dc.source.id SCOPUS0004640X-1984-100-12-SID34250135993


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  • Публикации сотрудников КФУ Scopus [24551]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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