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Abstract:

We study different approximations usually made to simplify the calculation of chromospheric models of M dwarf stars. The approximations we discuss in details are: the assumption that the minority species are in LTE, the omission of the contribution of numerous atomic and molecular lines (line blanketing) to the opacity, and the Complete Frequency Redistribution for the Lyα line. We consider a "cold" chromospheric model corresponding to a low activity dM star and a "hot" one corresponding to a very active dMe star. We find that the assumptions under study affect more strongly the cold than the hot model. In particular the approximation of Complete Frequency Redistribution in the Lyα line, through the statistical equilibrium and ionization equilibrium equation, changes the electron density in the high chromosphere and strongly affects other line profiles.

Registro:

Documento: Artículo
Título:Building reliable models of M dwarf chromospheres: The impact of the usual assumptions
Autor:Falchi, A.; Mauas, P.J.D.
Filiación:Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50155 Firenze, Italy
Inst. Astronomia Y Fis. del Espacio, CC 67, Suc. 28, 1428-Buenos Aires, Argentina
Palabras clave:Stars: atmospheres; Stars: chromosphere; Stars: late-type
Año:1998
Volumen:336
Número:1
Página de inicio:281
Página de fin:289
Título revista:Astronomy and Astrophysics
Título revista abreviado:Astron. Astrophys.
ISSN:00046361
CODEN:AAEJA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v336_n1_p281_Falchi

Referencias:

  • Allard, F., Hauschildt, P.H., (1995) ApJ, 445, p. 433
  • Anderson, L.S., (1989) ApJ, 339, p. 558
  • Andretta, V., Doyle, J.G., Byrne, P.B., (1997) A&A, 322, p. 266
  • Avrett, E.H., Loeser, R., (1984) Methods in Radiative Transfer, p. 341. , W. Kalkofen ed. Cambridge, Univ. Press
  • Avrett, E.H., Machado, M.E., Kurucz, R.L., (1986) The Lower Atmosphere of Solar Flares, p. 216. , D.F. Neidig, ed. NSO Summer Workshop, Sunspot, New Mexico
  • Brett, J.M., (1995) A&A, 295, p. 736
  • Carbon, D.F., (1984) Methods of Radiative Transfer, p. 395. , W. Kalkofen ed
  • Cram, L.E., Mullan, D.J., (1979) ApJ, 234, p. 579
  • Doyle, J.G., Mathioudakis, M., Andretta, V., Short, C.I., Jelinski, P., (1997) A&A, 318, p. 853
  • Eriksson, K., Linsky, J.L., Simon, T., (1983) ApJ, 272, p. 665
  • Giampapa, M.S., Worden, S.P., Linsky, J.L., (1982) ApJ, 258, p. 740
  • Houdebine, E.R., Doyle, J.G., (1994) A&A, 289, p. 169
  • Houdebine, E.R., Doyle, J.G., (1994) A&A, 289, p. 185
  • Houdebine, E.R., Doyle, J.G., Kościelecki, M., (1995) A&A, 294, p. 773
  • Houdebine, E.R., Mathioudakis, M., Doyle, J.G., Foing, B.H., (1996) A&A, 305, p. 209
  • Hubeny, I., Lites, B.W., (1995) ApJ, 455, p. 376
  • Konjevic, N., Dimitrijevic, M., Swiese, W.L., (1984) J. Phys. Chem. Ref. Data, 13, p. 649
  • Kurucz, R.L., (1991) Precision Photometry: Astrophysics of the Galaxy, , eds. A.G. Davis Philip, A.R. Upgren, and K.A. Janes, L. Davis Press, Schenectady
  • Lewis, E.L., McNamara, L.F., Michels, H.H., (1972) Sol. Phys., 23, p. 287
  • Luttermoser, D.G., Johnson, H.R., Eaton, J., (1994) ApJ, 422, p. 351
  • Mauas, P.J., Avrett, E.H., Loeser, R., (1988) ApJ, 330, p. 1008
  • Mauas, P.J., Falchi, A., (1994) A&A, 281, p. 129. , Paper I
  • Mauas, P.J., Falchi, A., (1996) A&A, 310, p. 245. , Paper II
  • Mauas, P.J., Falchi, A., Pasquini, L., Pallavicini, R., (1997) A&A, 326, p. 249. , Paper III
  • Mauas, P.J., Falchi, A., (1998) A&A, , in preparation
  • Monteiro, T.S., Danby, E.L., Cooper, I.L., Dickinson, A.S., Lewis, E.L., (1988) J.Phys.B, 21, p. 4165
  • Mould, J.R., (1976) A&A, 48, p. 443
  • Robinson, R.D., Cram, L.E., Giampapa, M.S., (1990) ApJS, 78, p. 891
  • Short, C.I., Doyle, J.G., (1997) A&A, 326, p. 287
  • Sutton, K., (1978) JQSRT, 20, p. 233
  • Thatcher, J.D., Robinson, R.D., Rees, D.E., (1991) MNRAS, 250, p. 14
  • Tripicchio, A., Severino, G., Covino, E., Terranegra, L., García López, J., (1997) A&A, 327, p. 681
  • Vernazza, J.E., Avrett, E.H., Loeser, R., (1981) ApJS, 45, p. 635
  • Woods, T.N., Rottman, G.J., White, O.R., Fontenla, J., Avrett, E.H., (1995) ApJ, 442, p. 898

Citas:

---------- APA ----------
Falchi, A. & Mauas, P.J.D. (1998) . Building reliable models of M dwarf chromospheres: The impact of the usual assumptions. Astronomy and Astrophysics, 336(1), 281-289.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v336_n1_p281_Falchi [ ]
---------- CHICAGO ----------
Falchi, A., Mauas, P.J.D. "Building reliable models of M dwarf chromospheres: The impact of the usual assumptions" . Astronomy and Astrophysics 336, no. 1 (1998) : 281-289.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v336_n1_p281_Falchi [ ]
---------- MLA ----------
Falchi, A., Mauas, P.J.D. "Building reliable models of M dwarf chromospheres: The impact of the usual assumptions" . Astronomy and Astrophysics, vol. 336, no. 1, 1998, pp. 281-289.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v336_n1_p281_Falchi [ ]
---------- VANCOUVER ----------
Falchi, A., Mauas, P.J.D. Building reliable models of M dwarf chromospheres: The impact of the usual assumptions. Astron. Astrophys. 1998;336(1):281-289.
Available from: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v336_n1_p281_Falchi [ ]