We have taken O, 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>2σ and χ2>1 were considered to be magnetic. The galactic coordinates and other parameters of all O, B, A, and F type stars were taken from SIMBAD. The spatial and surface densities of all considered types of stars were calculated.
Переведенное названиеПространственное распределения магнитных звезд ранних спектральных типов
Язык оригиналаАнглийский
Название основной публикацииSTARS: FROM COLLAPSE TO COLLAPSE
РедакторыYY Balega, DO Kudryavtsev, Romanyuk, IA Yakunin
ИздательAstronomical Society of the Pacific
Страницы270-271
Число страниц2
ISBN (печатное издание)978-1-58381-904-3
СостояниеОпубликовано - 2017
СобытиеConference on Stars: From Collapse to Collapse - Nizhny Arkhyz
Продолжительность: 2 окт 2016 → 6 окт 2016

Серия публикаций

НазваниеAstronomical Society of the Pacific Conference Series
ИздательASTRONOMICAL SOC PACIFIC
Том510

конференция

конференцияConference on Stars: From Collapse to Collapse
ГородNizhny Arkhyz
Период2/10/16 → 6/10/16

ID: 9366566