Spatial Distribution of Early Spectral Type Magnetic Stars

S. V. Boronina, A. F. Kholtygin

Research output: Chapter in Book/Report/Conference proceedingConference contributionResearchpeer-review

Abstract

We have taken 0, B, A and F magnetic stars from the catalog by Bychkov et. al. (2009) and divided them into three groups: stars with the rms magnetic field strength (B)(e) > 100G was accepted as "suspected to be magnetic". Some of the "suspected to be magnetic" stars satisfying both conditions (B)e > 2 sigma and X-2 > 1 were considered to be magnetic. The galactic coordinates and other parameters of all 0, B, A, and F type stars were taken from SIMBAD. The spatial and surface densities of all considered types of stars were calculated.

Translated title of the contributionПространственное распределения магнитных звезд ранних спектральных типов
Original languageEnglish
Title of host publicationSTARS: FROM COLLAPSE TO COLLAPSE
EditorsYY Balega, DO Kudryavtsev, Romanyuk, IA Yakunin
PublisherAstronomical Society of the Pacific
Pages270-271
Number of pages2
ISBN (Print)978-1-58381-904-3
StatePublished - 2017
EventConference on Stars: From Collapse to Collapse - Nizhny Arkhyz
Duration: 2 Oct 20166 Oct 2016

Publication series

NameAstronomical Society of the Pacific Conference Series
PublisherASTRONOMICAL SOC PACIFIC
Volume510

Conference

ConferenceConference on Stars: From Collapse to Collapse
CityNizhny Arkhyz
Period2/10/166/10/16

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