M. Pavlović, A. Dobardžić, B. Vukoti'c, D. Urošević
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引用次数: 31
Abstract
In this paper we present the updated empirical radio surface-
brightness-to-diameter (?-D) relation for Galactic supernova remnants (SNRs)
calibrated using 110 SNRs with reliable distances. We apply orthogonal
fitting procedure and kernel density smoothing in the ? ? D plane and compare
the results with the latest theoretical ? - D relations derived from
simulations of radio evolution of SNRs. We argue that the best agreement
between the empirical and simulated ? ? D relations is achieved if the
mixed-morphology SNRs and SNRs of both, low brightness and small diameter,
are filtered out from the calibration sample. The distances to 5 newly
discovered remnants and 27 new candidates for shell SNRs are estimated from
our full and filtered calibration samples.
期刊介绍：
Serbian Astronomical Journal publishes original observations and researches in all branches of astronomy. The journal publishes:
Invited Reviews - review article on some up-to-date topic in astronomy, astrophysics and related fields (written upon invitation only),
Original Scientific Papers - article in which are presented previously unpublished author''s own scientific results,
Preliminary Reports - original scientific paper, but shorter in length and of preliminary nature,
Professional Papers - articles offering experience useful for the improvement of professional practice i.e. article describing methods and techniques, software, presenting observational data, etc.
In some cases the journal may publish other contributions, such as In Memoriam notes, Obituaries, Book Reviews, as well as Editorials, Addenda, Errata, Corrigenda, Retraction notes, etc.
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