Artículo

Schneiter, E.M.; Velázquez, P.F.; Reynoso, E.M.; De Colle, F. "An MHD study of SN 1006 and determination of the ambient magnetic field direction" (2010) Monthly Notices of the Royal Astronomical Society. 408(1):430-435
Estamos trabajando para incorporar este artículo al repositorio
Consulte el artículo en la página del editor
Consulte la política de Acceso Abierto del editor

Abstract:

In this work, we employ a magnetohydrodynamic (MHD) numerical code to reproduce the morphology observed for SN 1006 in radio synchrotron and thermal X-ray emission. We introduce a density discontinuity, in the form of a flat cloud parallel to the Galactic plane, in order to explain the NW filament observed in optical wavelengths and in thermal X-rays. We compare our models with observations. We also perform a test that contrasts the radio emitting bright limbs of the supernova remnant against the central region, finding additional support to our results. Our main conclusion is that the most probable direction of the ambient magnetic field is on average perpendicular to the Galactic plane. © 2010 The Authors. Journal compilation © 2010 RAS.

Registro:

Documento: Artículo
Título:An MHD study of SN 1006 and determination of the ambient magnetic field direction
Autor:Schneiter, E.M.; Velázquez, P.F.; Reynoso, E.M.; De Colle, F.
Filiación:Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, México D.F., Mexico
Instituto de Astronomía y Física del Espacio, Ciudad Universitaria, C.C. 67, C.P. 1428, Buenos Aires, Argentina
Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, United States
Palabras clave:ISM: supernova remnants; Methods: numerical; MHD; Radiation mechanisms: general; Supernovae: individual: SN 1006
Año:2010
Volumen:408
Número:1
Página de inicio:430
Página de fin:435
DOI: http://dx.doi.org/10.1111/j.1365-2966.2010.17125.x
Título revista:Monthly Notices of the Royal Astronomical Society
Título revista abreviado:Mon. Not. R. Astron. Soc.
ISSN:00358711
CODEN:MNRAA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v408_n1_p430_Schneiter

Referencias:

  • Acero, F., Ballet, J., Decourchelle, A., (2007) A&A, 475, p. 883
  • Bell, A.R., (2004) MNRAS, 353, p. 550
  • Blandford, R., Eichler, D., (1987) Phys. Rept., 154, p. 1
  • Cassam-Chenaï, G., Hughes, J.P., Reynoso, E.M., Badenes, C., Moffett, D., (2008) ApJ, 680, p. 1180
  • Dalgarno, A., McCray, R.A., (1972) ARA&A, 10, p. 375
  • De Colle, F., (2005), PhD. thesis, IA-UNAM; De Colle, F., Raga, A.C., (2005) MNRAS, 359, p. 164
  • De Colle, F., Raga, A.C., (2006) A&A, 449, p. 1061
  • Dere, K.P., Landi, E., Mason, H.E., Monsignori Fossi, B.C., Young, P.R., (1997) A&AS, 125, p. 149
  • Dubner, G.M., Giacani, E.B., Goss, W.M., Green, A.J., Nyman L.Å, (2002) A&A, 387, p. 1047
  • Fulbright, M.S., Reynolds, S.P., (1990) ApJ, 357, p. 591
  • Gaensler, B.M., (1998) ApJ, 493, p. 781
  • Ginzburg, V.L., Syrovatskii, S.I., (1965) ARA&A, 3, p. 297
  • Harten, A., Lax, P., Van Leer, B., (1983) SIAM Rev., 25, p. 35
  • Jun, B.I., Jones, T.W., Norman, M.L., (1996) ApJ, 468, pp. L59
  • Jokipii, J.R., (1987) ApJ, 313, p. 842
  • Kesteven, M.J., Caswell, J.L., (1987) A&A, 183, p. 118
  • Landi, E., Phillips, K.J.H., (2006) ApJS, 166, p. 421
  • Mazzotta, P., Mazzitelli, G., Colafrancesco, S., Vittorio, N., (1998) A&AS, 133, p. 403
  • Miceli, M., (2009) A&A, 501, p. 239
  • Morrison, R., McCammon, D., (1983) ApJ, 270, p. 119
  • Orlando, S., Bocchino, F., Reale, F., Peres, G., Petruk, O., (2007) A&A, 470, p. 927
  • Petruk, O., (2009) MNRAS, 393, p. 1034
  • Rakowski, C.E., Laming, J.M., Ghavamian, P., (2008) ApJ, 684, p. 348
  • Rothenflug, R., Ballet, J., Dubner, G., Giacani, E., Decourchelle, A., Ferrando, P., (2004) A&A, 425, p. 121
  • Truelove, J.K., McKee, C.F., (1999) ApJS, 120, p. 299
  • Tóth, G., (2000) J. Comput. Phys., 161, p. 605
  • Völk, H.J., Berezhko, E.G., Ksenofontov, L.T., (2003) A&A, 409, p. 563

Citas:

---------- APA ----------
Schneiter, E.M., Velázquez, P.F., Reynoso, E.M. & De Colle, F. (2010) . An MHD study of SN 1006 and determination of the ambient magnetic field direction. Monthly Notices of the Royal Astronomical Society, 408(1), 430-435.
http://dx.doi.org/10.1111/j.1365-2966.2010.17125.x
---------- CHICAGO ----------
Schneiter, E.M., Velázquez, P.F., Reynoso, E.M., De Colle, F. "An MHD study of SN 1006 and determination of the ambient magnetic field direction" . Monthly Notices of the Royal Astronomical Society 408, no. 1 (2010) : 430-435.
http://dx.doi.org/10.1111/j.1365-2966.2010.17125.x
---------- MLA ----------
Schneiter, E.M., Velázquez, P.F., Reynoso, E.M., De Colle, F. "An MHD study of SN 1006 and determination of the ambient magnetic field direction" . Monthly Notices of the Royal Astronomical Society, vol. 408, no. 1, 2010, pp. 430-435.
http://dx.doi.org/10.1111/j.1365-2966.2010.17125.x
---------- VANCOUVER ----------
Schneiter, E.M., Velázquez, P.F., Reynoso, E.M., De Colle, F. An MHD study of SN 1006 and determination of the ambient magnetic field direction. Mon. Not. R. Astron. Soc. 2010;408(1):430-435.
http://dx.doi.org/10.1111/j.1365-2966.2010.17125.x