期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 487, 期 3, 页码 3904-3913出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz1545
关键词
stars: early-type; stars: evolution; stars: magnetic fields; stars: massive
资金
- Delaware Space Grant
- National Science Foundation [1747658]
- University of Delaware Research Foundation
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1747658] Funding Source: National Science Foundation
It has been suggested that the absence of macroturbulence in the atmosphere of NGC 1624-2 is due its strong magnetic field (the strongest known for a massive O star) suppressing convection in its outer layers, removing the mechanism thought responsible for the observed macroturbulence in stars with lower field strengths. Here, we develop and apply a criterion for a uniform magnetic field to suppress convection in stellar envelopes in which radiation pressure is a significant contributor to hydrostatic balance. We find upper mass limits of similar to 55 and similar to 30 M-circle dot for magnetic suppression to be possible in zero-age main-sequence and terminal-age main-sequence stars, respectively. For evolved stars, magnetic suppression of convection can significantly alter the stars' evolution. For NGC 1624-2, we find that a polar dipole strength of 16.5 +/- 5.9 kG is required to suppress convection, in good agreement with the value similar to 20 kG measured by spectropolarimetry.
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