Reconstructing the Extreme Ultraviolet Emission of Cool Dwarfs Using Differential Emission Measure Polynomials

Characterizing the atmospheres of planets orbiting M dwarfs requires understanding the spectral energy distributions of M dwarfs over planetary lifetimes. Surveys like MUSCLES, HAZMAT, and FUMES have collected multiwavelength spectra across the spectral type’s range of T eff and activity, but the ex...

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Veröffentlicht in:	The Astrophysical journal 2021-05, Vol.913 (1), p.40
Hauptverfasser:	Duvvuri, Girish M., Sebastian Pineda, J., Berta-Thompson, Zachory K., Brown, Alexander, France, Kevin, Kowalski, Adam F., Redfield, Seth, Tilipman, Dennis, Vieytes, Mariela C., Wilson, David J., Youngblood, Allison, Froning, Cynthia S., Linsky, Jeffrey, Parke Loyd, R. O., Mauas, Pablo, Miguel, Yamila, Newton, Elisabeth R., Rugheimer, Sarah, Christian Schneider, P.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Atmospheric evolution Emission lines Emission measurements Extrasolar planets Fluctuations Flux Fumes Hazardous materials Hubble Space Telescope Interstellar chemistry Interstellar matter Interstellar medium Low mass stars M dwarf stars Muscles Occultation Planetary atmospheres Planetary evolution Polynomials Red dwarf stars Solar extreme ultraviolet emission Space telescopes Stellar activity Stellar atmospheres Stellar chromospheres Stellar coronae Thermosphere Ultraviolet astronomy Ultraviolet emission Uncertainty X ray spectra X ray telescopes XMM (spacecraft)
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