Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Matt E. Shultz"'
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 2, p 152 (2023)
Although the majority of hot magnetic stars have extremely stable, ∼kilogauss strength surface magnetic fields with simple topologies, a subset undergoes small-scale explosions due to centrifugal breakout. The resulting small-scale flares are typic
Externí odkaz:
https://doaj.org/article/60face89c6a24730ad63f64bcc95a42d
Autor:
Barnali Das, Poonam Chandra, Matt E Shultz, Paolo Leto, Zdeněk Mikulášek, Véronique Petit, Gregg A Wade
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 517:5756-5769
Coherent radio emission via electron cyclotron maser emission (ECME) from hot magnetic stars was discovered more than two decades ago, but the physical conditions that make the generation of ECME favourable remain uncertain. Only recently was an empi
Autor:
Barnali Das, Poonam Chandra, Matt E. Shultz, Gregg A. Wade, James Sikora, Oleg Kochukhov, Coralie Neiner, Mary E. Oksala, Evelyne Alecian
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, In press
HAL
The Astrophysical Journal, American Astronomical Society, In press
HAL
'Main-sequence radio pulse-emitters' (MRPs) are magnetic early-type stars from which periodic radio pulses, produced via electron cyclotron maser emission (ECME), are observed. Despite the fact that these stars can naturally offer suitable conditions
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54cd3b6b6648079e379b4c1222b4a4d3
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 497:L67-L68
Publikováno v:
Astrophysical Journal; Jun2019, Vol. 877 Issue 2, p1-1, 1p