Artículo

Orio, M.; Behar, E.; Gallagher, J.; Bianchini, A.; Chiosi, E.; Luna, G.J.M.; Nelson, T.; Rauch, T.; Schaefer, B.E.; Tofflemire, B. "Thomson scattering and collisional ionization in the X-ray grating spectra of the recurrent nova U Scorpii" (2013) Monthly Notices of the Royal Astronomical Society. 429(2):1342-1353
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:

We present a Chandra observation of the recurrent nova U Scorpii, done with the High Resolution camera-S (HRC-S) detector and the Low Energy Transmission Grating (LETG) on day 18 after the observed visual maximum of 2010, and compare it with XMM-Newton observations obtained on days 23 and 35 after maximum. The total absorbed flux was in the range 2.2-2.6 × 10 -11 erg cm -2 s -1 , corresponding to unabsorbed luminosity 7-8.5 × 10 36 ×(d/12 kpc) 2 for N(H) = 2-2.7 × 10 21 cm -2 . On day 18, 70 per cent of the soft X-tray flux was in a continuum typical of a very hot white dwarf (WD) atmosphere, which accounted for about 80 per cent of the flux on days 23 and 35. In addition, all spectra display very broad emission lines, due to higher ionization stages at later times. With Chandra we observed apparent P Cygni profiles. We find that these peculiar profiles are not due to blueshifted absorption and redshifted emission in photoionized ejecta, like the optical P Cyg of novae, but they are rather a superposition of WD atmospheric absorption features reflected by the already discovered Thomson scattering corona, and emission lines due to collisional ionization in condensations in the ejecta. On days 23 and 35, the absorption components were no longer measurable, having lost the initial large blueshift that displaced them from the core of the broad emission lines. We interpret this as an indication that mass-loss ceased between day 18 and day 23. On day 35, the emission line spectrum became very complex, with several different components. Model atmospheres indicate that theWD atmospheric temperature was about 730 000 K on day 18 and reached 900 000-1000 000 K on day 35. This peak temperature is consistent with a WD mass of at least 1.3 M⊙. © 2012 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.

Registro:

Documento: Artículo
Título:Thomson scattering and collisional ionization in the X-ray grating spectra of the recurrent nova U Scorpii
Autor:Orio, M.; Behar, E.; Gallagher, J.; Bianchini, A.; Chiosi, E.; Luna, G.J.M.; Nelson, T.; Rauch, T.; Schaefer, B.E.; Tofflemire, B.
Filiación:INAF - Osservatorio di Padova, Vicolo dell-Osservatorio 5, I-35122 Padova, Italy
Department of Astronomy, University of Wisconsin, 475 N. Charter Str., Madison, WI 53704, United States
Department of Physics, Technion, Haifa 32000, Israel
Astronomy Department, Padova University, Vicolo dell' Osservatorio 3, I-35122 Padova, Italy
Instituto de Astronom'ia y Fisica del Espacio (IAFE/Conicet), CC67, Suc. 28 C1428ZAA CABA, Argentina
School of Physics and Astronomy, University of Minnesota, 116 Church St SE, Minneapolis, MN 55455, United States
Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, D-72076 Tubingen, Germany
Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803, United States
Palabras clave:Binaries-X-rays; Cataclysmic variables-white dwarfs-stars; Individual; Stars; U Scorpii; U Scorpii-novae; Winds-outflows-X-rays
Año:2013
Volumen:429
Número:2
Página de inicio:1342
Página de fin:1353
DOI: http://dx.doi.org/10.1093/mnras/sts421
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_v429_n2_p1342_Orio

Referencias:

  • Anupama, G.C., Dewangan, G.C., (2000) AJ, 119, p. 1359
  • Balman, S., Krautter, J., Ögelman, H., (1998) ApJ, 499, p. 345
  • Barlow, M.J., (1981) MNRAS, 195, p. 61
  • Behar, E., Leutenegger, M., Doron, R., G̈udel, M., Feldman, U., Audard, M., Kahn, S.M., (2004) ApJ, 612, pp. L65
  • Brinkman, A.C., (2000) ApJ, 530, pp. L111
  • Cash, W., (1979) ApJ, 228, p. 939
  • Chen, H., Beiersdorfer, P., Heeter, L.A., Liedahl, D.A., Naranjo-Rivera, K.L., Tr̈abert, E., Gu, M.F., Lepson, J.K., (2004) ApJ, 611, p. 298
  • Drake, J.J., (2003) ApJ, 584, p. 548
  • D̈urbeck, H.W., D̈ummler, R., Seitter, W.C., Leibowitz, E.M., Shara, M.M., (2003) The Messenger, 71, p. 19
  • Gabriel, A.H., Jordan, C., (1969) MNRAS, 145, p. 241
  • Gallagher, J.S., Anderson, C.M., (1976) ApJ, 203, p. 625
  • Hachisu, I., Kato, M., (2010) ApJ, 709, p. 680
  • Kahabka, P., Hartmann, H.W., Parmar, A.N., Neguerela, I., (1999) A&A, 347, pp. L43
  • Kinkhabwala, A., (2002) ApJ, 575, p. 732
  • Lloyd, H.M., O'Brien, T.J., Bode, M.F., Predehl, P., Schmitt, J.H.M.M., Truemper, J., Watson, M.G., Pounds, K.A., (1992) Nat, 350, p. 222
  • Mason, E., Ederoclite, A., Williams, R.E., Della Valle, M., Setiawan, J., (2012) A&A, 544, p. 149
  • Maxwell, M.P., (2012) MNRAS, 419, p. 1465
  • Mukai, K., Kinkhabwala, A., Peterson, J.R., Kahn, S.M., Paerels, F., (2003) ApJ, 582, p. 184
  • Mukai, K., Orio, M., (2005) ApJ, 622, p. 602
  • Neff, J.S., Smith, V.V., Katelsen, D.A., (1978) ApJS, 38, p. 98
  • Nelson, T., Orio, M., Cassinelli, J.P., Still, M., Leibowitz, E., Mucciarelli, P., (2008) ApJ, 673, p. 1067
  • Ness, J.-U., (2001) A&A, 367, p. 282
  • Ness, J.-U., Brickhouse, N.S., Drake, J.J., Huenemoerder, D.P., (2003) ApJ, 598, p. 1289
  • Ness, J.-U., (2011) Presentations of a Conference held in Berlin, , 27-30 June 2011, The X-ray Universe 2011
  • Ness, J.-U., (2011) ApJ, 733, p. 70
  • Ness, J.-U., (2012) ApJ, 745, p. 43
  • O'Brien, T.J., Lloyd, H.M., (1994) MNRAS, 271, p. 155
  • Orio, M., Nelson, T., Gallagher, J., (2011) HEAD Meeting, , 12.11.06
  • Orio, M., Binary Paths to Type Ia Supernovae Explosions (2012) Di Stefano R., Moe M., Orio M., eds, Cambridge Univ. Press, Cambridge, in press
  • Orio, M., Hartmann, W., Still, M., Greiner, J., (2003) ApJ, 594, p. 435
  • Orio, M., Ebisawa, K., Heise, J., Hartmann, J., (2004) Revista Mexicana de Astronomia y Astrofisica, 610, p. 194
  • Pinto, C., (2012) A&A, 543, p. 134
  • Rauch, T., Orio, M., Gonzales-Riestra, R., Nelson, T., Still, M., Werner, K., Wilms, J., (2010) ApJ, 717, p. 363
  • Schaefer, B.E., (1990) ApJ, 355, pp. L39
  • Schaefer, B.E., (2011) ApJ, 742, p. 112
  • Schaefer, B.E., Ringwald, F.A., (1995) ApJ, 447, pp. L45
  • Schaefer, B., (2010) AJ, 140, p. 925
  • Schaefer, B., (2011) ApJ, 472, p. 113
  • Starrfield, S., Sparks, W.M., Shaviv, G., (1988) ApJ, 325, pp. L35
  • Thoroughgood, T.D., (2001) MNRAS, 327, p. 1323
  • Tofflemire, B., Orio, M., (2012) preprint
  • Yamanaka, M., (2010) PASJ, 62, pp. L37
  • Yaron, O., Prialnik, D., Shara, M.M., Kovetz, A., (2005) ApJ, 623, p. 398

Citas:

---------- APA ----------
Orio, M., Behar, E., Gallagher, J., Bianchini, A., Chiosi, E., Luna, G.J.M., Nelson, T.,..., Tofflemire, B. (2013) . Thomson scattering and collisional ionization in the X-ray grating spectra of the recurrent nova U Scorpii. Monthly Notices of the Royal Astronomical Society, 429(2), 1342-1353.
http://dx.doi.org/10.1093/mnras/sts421
---------- CHICAGO ----------
Orio, M., Behar, E., Gallagher, J., Bianchini, A., Chiosi, E., Luna, G.J.M., et al. "Thomson scattering and collisional ionization in the X-ray grating spectra of the recurrent nova U Scorpii" . Monthly Notices of the Royal Astronomical Society 429, no. 2 (2013) : 1342-1353.
http://dx.doi.org/10.1093/mnras/sts421
---------- MLA ----------
Orio, M., Behar, E., Gallagher, J., Bianchini, A., Chiosi, E., Luna, G.J.M., et al. "Thomson scattering and collisional ionization in the X-ray grating spectra of the recurrent nova U Scorpii" . Monthly Notices of the Royal Astronomical Society, vol. 429, no. 2, 2013, pp. 1342-1353.
http://dx.doi.org/10.1093/mnras/sts421
---------- VANCOUVER ----------
Orio, M., Behar, E., Gallagher, J., Bianchini, A., Chiosi, E., Luna, G.J.M., et al. Thomson scattering and collisional ionization in the X-ray grating spectra of the recurrent nova U Scorpii. Mon. Not. R. Astron. Soc. 2013;429(2):1342-1353.
http://dx.doi.org/10.1093/mnras/sts421