NGTS clusters survey – II. White-light flares from the youngest stars in Orion
Autor: | Christopher A. Watson, Samuel Gill, Maximiliano Moyano, Claudia Belardi, Michael R. Goad, Sarah L. Casewell, Richard G. West, James McCormac, Liam Raynard, Peter J. Wheatley, David R. Anderson, Matthew R. Burleigh, Jack S. Acton, James S. Jenkins, Simon Hodgkin, Philipp Eigmüller, Rosanna H. Tilbrook, James A. G. Jackman, Edward Gillen, Andrew Grange, Didier Queloz |
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Přispěvatelé: | Apollo - University of Cambridge Repository, Queloz, Didier [0000-0002-3012-0316] |
Rok vydání: | 2020 |
Předmět: |
Extrasolare Planeten und Atmosphären
endocrine system astro-ph.SR Astrophysics::High Energy Astrophysical Phenomena FOS: Physical sciences Library science stars: pre-main-sequence Astrophysics::Cosmology and Extragalactic Astrophysics 01 natural sciences Queen (playing card) stars: low-mass 0103 physical sciences White light Astrophysics::Solar and Stellar Astrophysics skin and connective tissue diseases 010303 astronomy & astrophysics Solar and Stellar Astrophysics (astro-ph.SR) Astrophysics::Galaxy Astrophysics Earth and Planetary Astrophysics (astro-ph.EP) Physics 010308 nuclear & particles physics Astronomy and Astrophysics Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science astro-ph.EP Physics::Space Physics stars: flare Administration (government) Astrophysics - Earth and Planetary Astrophysics |
Zdroj: | Jackman, J A G, Wheatley, P J, Acton, J S, Anderson, D R, Belardi, C, Burleigh, M R, Casewell, S L, Eigmüller, P, Gill, S, Gillen, E, Goad, M R, Grange, A, Hodgkin, S T, Jenkins, J S, McCormac, J, Moyano, M, Queloz, D, Raynard, L, Tilbrook, R H, Watson, C A & West, R G 2020, ' NGTS clusters survey--II. White-light flares from the youngest stars in Orion ', Monthly Notices of the Royal Astronomical Society . https://doi.org/10.1093/mnras/staa1971 |
ISSN: | 1365-2966 0035-8711 |
Popis: | We present the detection of high energy white-light flares from pre-main sequence stars associated with the Orion complex, observed as part of the Next Generation Transit Survey (NGTS). With energies up to $5.2\times10^{35}$ erg these flares are some of the most energetic white-light flare events seen to date. We have used the NGTS observations of flaring and non-flaring stars to measure the average flare occurrence rate for 4 Myr M0-M3 stars. We have also combined our results with those from previous studies to predict average rates for flares above $1\times10^{35}$ ergs for early M stars in nearby young associations. Comment: 10 pages, 5 figures, 5 tables. Accepted for publication in the Monthly Notices of the Royal Astronomical Society |
Databáze: | OpenAIRE |
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