Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Research › peer-review
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 contribution | Пространственное распределения магнитных звезд ранних спектральных типов |
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Original language | English |
Title of host publication | STARS: FROM COLLAPSE TO COLLAPSE |
Editors | YY Balega, DO Kudryavtsev, Romanyuk, IA Yakunin |
Publisher | Astronomical Society of the Pacific |
Pages | 270-271 |
Number of pages | 2 |
ISBN (Print) | 978-1-58381-904-3 |
State | Published - 2017 |
Event | Conference on Stars: From Collapse to Collapse - Nizhny Arkhyz Duration: 2 Oct 2016 → 6 Oct 2016 |
Name | Astronomical Society of the Pacific Conference Series |
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Publisher | ASTRONOMICAL SOC PACIFIC |
Volume | 510 |
Conference | Conference on Stars: From Collapse to Collapse |
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City | Nizhny Arkhyz |
Period | 2/10/16 → 6/10/16 |
ID: 9366566