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Abstract:

Stellar radiation from X-rays to the visible provides the energy that controls the photochemistry and mass loss from exoplanet atmospheres. The important extreme ultraviolet (EUV) region (10-91.2 nm) is inaccessible and should be computed from a reliable stellar model. It is essential to understand the formation regions and physical processes responsible for the various stellar emission features to predict how the spectral energy distribution varies with age and activity levels. We compute a state-of-the-art semi-empirical atmospheric model and the emergent high-resolution synthetic spectrum of the moderately active M2 V star GJ 832 as the first of a series of models for stars with different activity levels. We construct a one-dimensional simple model for the physical structure of the star's chromosphere, chromosphere-corona transition region, and corona using non-LTE radiative transfer techniques and many molecular lines. The synthesized spectrum for this model fits the continuum and lines across the UV-to-optical spectrum. Particular emphasis is given to the emission lines at wavelengths that are shorter than 300 nm observed with the Hubble Space Telescope, which have important effects on the photochemistry of the exoplanet atmospheres. The FUV line ratios indicate that the transition region of GJ 832 is more biased to hotter material than that of the quiet Sun. The excellent agreement of our computed EUV luminosity with that obtained by two other techniques indicates that our model predicts reliable EUV emission from GJ 832. We find that the unobserved EUV flux of GJ 832, which heats the outer atmospheres of exoplanets and drives their mass loss, is comparable to the active Sun. © 2016. The American Astronomical Society. All rights reserved.

Registro:

Documento: Artículo
Título:SEMI-EMPIRICAL MODELING of the PHOTOSPHERE, CHROMOPSHERE, TRANSITION REGION, and CORONA of the M-DWARF HOST STAR GJ 832
Autor:Fontenla, J.M.; Linsky, J.L.; Witbrod, J.; France, K.; Buccino, A.; Mauas, P.; Vieytes, M.; Walkowicz, L.M.
Filiación:NorthWest Research Associates, Boulder, CO 80301, United States
JILA, University of Colorado, NIST, Boulder, CO 80309-0440, United States
University of Colorado, Boulder, CO 80309, United States
LASP, University of Colorado, Boulder, CO 80309-0600, United States
Instituto de Astronomía y Física Del Espacio (CONICET-UBA), C.C. 67, Sucursal 28, Buenos Aires, C1428EHA, Argentina
Adler Planetarium, Chicago, IL 60605, United States
Palabras clave:planet-star interactions; stars: chromospheres; stars: coronae; stars: individual (GJ 832); stars: late-type; ultraviolet: stars
Año:2016
Volumen:830
Número:2
DOI: http://dx.doi.org/10.3847/0004-637X/830/2/154
Título revista:Astrophysical Journal
Título revista abreviado:Astrophys. J.
ISSN:0004637X
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v830_n2_p_Fontenla

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Citas:

---------- APA ----------
Fontenla, J.M., Linsky, J.L., Witbrod, J., France, K., Buccino, A., Mauas, P., Vieytes, M.,..., Walkowicz, L.M. (2016) . SEMI-EMPIRICAL MODELING of the PHOTOSPHERE, CHROMOPSHERE, TRANSITION REGION, and CORONA of the M-DWARF HOST STAR GJ 832. Astrophysical Journal, 830(2).
http://dx.doi.org/10.3847/0004-637X/830/2/154
---------- CHICAGO ----------
Fontenla, J.M., Linsky, J.L., Witbrod, J., France, K., Buccino, A., Mauas, P., et al. "SEMI-EMPIRICAL MODELING of the PHOTOSPHERE, CHROMOPSHERE, TRANSITION REGION, and CORONA of the M-DWARF HOST STAR GJ 832" . Astrophysical Journal 830, no. 2 (2016).
http://dx.doi.org/10.3847/0004-637X/830/2/154
---------- MLA ----------
Fontenla, J.M., Linsky, J.L., Witbrod, J., France, K., Buccino, A., Mauas, P., et al. "SEMI-EMPIRICAL MODELING of the PHOTOSPHERE, CHROMOPSHERE, TRANSITION REGION, and CORONA of the M-DWARF HOST STAR GJ 832" . Astrophysical Journal, vol. 830, no. 2, 2016.
http://dx.doi.org/10.3847/0004-637X/830/2/154
---------- VANCOUVER ----------
Fontenla, J.M., Linsky, J.L., Witbrod, J., France, K., Buccino, A., Mauas, P., et al. SEMI-EMPIRICAL MODELING of the PHOTOSPHERE, CHROMOPSHERE, TRANSITION REGION, and CORONA of the M-DWARF HOST STAR GJ 832. Astrophys. J. 2016;830(2).
http://dx.doi.org/10.3847/0004-637X/830/2/154