Navegar

Colección

Datos Estadísticas

Artículo

Miceli, M.; Orlando, S.; Pereira, V.; Acero, F.; Katsuda, S.; Decourchelle, A.; Winkler, F.P.; Bonito, R.; Reale, F.; Peres, G.; Li, J.; Dubner, G. "Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission" (2016) Astronomy and Astrophysics. 593
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:

Context. The supernova remnant SN 1006 is a source of high-energy particles and its southwestern limb is interacting with a dense ambient cloud, thus is a promising region for γ-ray hadronic emission. Aims. We aim at describing the physics and the nonthermal emission associated with the shock-cloud interaction to derive the physical parameters of the cloud (poorly constrained by the data analysis), to ascertain the origin of the observed spatial variations in the spectral properties of the X-ray synchrotron emission, and to predict spectral and morphological features of the resulting γ-ray emission. Methods. We performed 3D magnetohydrodynamic simulations modeling the evolution of SN 1006 and its interaction with the ambient cloud, and explored different model setups. By applying the REMLIGHT code on the model results, we synthesized the synchrotron X-ray emission and compared it with actual observations to constrain the parameters of the model. We also synthesized the leptonic and hadronic γ-ray emission from the models, deriving constraints on the energy content of the hadrons accelerated at the southwestern limb. Results. We found that the impact of the SN 1006 shock front with a uniform cloud with density 0.5 cm -3 can explain the observed morphology, the azimuthal variations of the cutoff frequency of the X-ray synchrotron emission, and the shock proper motion in the interaction region. Our results show that the current upper limit for the total hadronic energy in the southwestern limb is 2.5 × 10 49 erg. © 2016 ESO.

Registro:

Documento: Artículo
Título:Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission
Autor:Miceli, M.; Orlando, S.; Pereira, V.; Acero, F.; Katsuda, S.; Decourchelle, A.; Winkler, F.P.; Bonito, R.; Reale, F.; Peres, G.; Li, J.; Dubner, G.
Filiación:Dipartimento di Fisica, Chimica Università di Palermo, Piazza del Parlamento 1, Palermo, 90134, Italy
INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, Palermo, 90134, Italy
Dpto. de Astrofísica y CC de la Atmósfera, Universidad Complutense de Madrid, Madrid, 28040, Spain
Laboratoire AIM, CEA-IRFU, Université Paris Diderot, Gif-sur-Yvette, 91191, France
Department of Physics, Faculty of Science and Engineering, Chuo University, 1-13-27 Kasuga, Bunkyo, Tokyo, 112-8551, Japan
Service d'Astrophysique, CEA Saclay, Gif-sur-Yvette Cedex, 91191, France
Department of Physics, Middlebury College, Middlebury, VT 05753, United States
Department of Astronomy, University of Michigan, 311 West Hall, Ann Arbor, MI 48109-1107, United States
Instituto de Astronomiá y Física Del Espacio (IAFE), UBA-CONICET, CC 67, Buenos Aires, 1428, Argentina
Palabras clave:Acceleration of particles; ISM: clouds; ISM: individual objects: SN 1006; ISM: supernova remnants; Magnetohydrodynamics (MHD); X-rays: ISM; Cutoff frequency; Magnetohydrodynamics; Supernovae; Synchrotron radiation; Acceleration of particles; ISM : clouds; Ism: individual objects: sn 1006; ISM: supernova remnants; X rays: ISM; Gamma rays
Año:2016
Volumen:593
DOI: http://dx.doi.org/10.1051/0004-6361/201628725
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_v593_n_p_Miceli

Referencias:

  • Acero, F., Ballet, J., Decourchelle, A., (2007) A&A, 475, p. 883
  • Acero, F., Aharonian, F., Akhperjanian, A.G., (2010) A&A, 516, p. A62
  • Acero, F., Lemoine-Goumard, M., Renaud, M., (2015) A&A, 580, p. A74
  • Amato, E., Blasi, P., (2006) MNRAS, 371, p. 1251
  • Berezhko, E.G., Ksenofontov, L.T., Völk, H.J., (2012) ApJ, 759, p. 12
  • Blasi, P., (2002) Astropart. Phys., 16, p. 429
  • Blasi, P., (2004) Astropart. Phys., 21, p. 45
  • Bocchino, F., Orlando, S., Miceli, M., Petruk, O., (2011) A&A, 531, p. A129
  • Broersen, S., Vink, J., Miceli, M., (2013) A&A, 552, p. A9
  • Bykov, A.M., Ellison, D.C., Renaud, M., (2012) Space Sci. Rev., 166, p. 71
  • Caprioli, D., (2012) J. Cosmol. Astropart. Phys., 7, p. 038
  • Chevalier, R.A., (1982) ApJ, 258, p. 790
  • Ferrand, G., Decourchelle, A., Ballet, J., Teyssier, R., Fraschetti, F., (2010) A&A, 509, p. L10
  • Ferrand, G., Decourchelle, A., Safi-Harb, S., (2014) ApJ, 789, p. 49
  • Fryxell, B., Olson, K., Ricker, P., (2000) ApJS, 131, p. 273
  • Ghavamian, P., Winkler, P.F., Raymond, J.C., Long, K.S., (2002) ApJ, 572, p. 888
  • Green, D.A., (2009) Bull. Astron. Soc. India, 37, p. 45
  • Kang, H., Jones, T.W., Edmon, P.P., (2013) ApJ, 777, p. 25
  • Katsuda, S., Petre, R., Long, K.S., (2009) ApJ, 692, p. L105
  • Katsuda, S., Petre, R., Mori, K., (2010) ApJ, 723, p. 383
  • Katsuda, S., Long, K.S., Petre, R., (2013) ApJ, 763, p. 85
  • Kelner, S.R., Aharonian, F.A., Bugayov, V.V., (2006) Phys. Rev. D, 74, p. 034018
  • Lee, S.-H., Ellison, D.C., Nagataki, S., (2012) ApJ, 750, p. 156
  • Li, J.-T., Decourchelle, A., Miceli, M., Vink, J., Bocchino, F., (2015) MNRAS, 453, p. 3953
  • Miceli, M., Bocchino, F., Iakubovskyi, D., (2009) A&A, 501, p. 239
  • Miceli, M., Bocchino, F., Decourchelle, A., (2012) A&A, 546, p. A66
  • Miceli, M., Bocchino, F., Decourchelle, A., (2013) A&A, 556, p. A80. , a
  • Miceli, M., Orlando, S., Reale, F., Bocchino, F., Peres, G., (2013) MNRAS, 430, p. 2864
  • Miceli, M., Acero, F., Dubner, G., (2014) ApJ, 782, p. L33
  • Miceli, M., Bocchino, F., Decourchelle, A., (2014) Astron. Nachr., 335, p. 252
  • Morlino, G., Amato, E., Blasi, P., Caprioli, D., (2010) MNRAS, 405, p. L21
  • Nikolić, S., Van De Ven, G., Heng, K., (2013) Science, 340, p. 45
  • Orlando, S., Bocchino, F., Reale, F., Peres, G., Petruk, O., (2007) A&A, 470, p. 927
  • Orlando, S., Petruk, O., Bocchino, F., Miceli, M., (2011) A&A, 526, p. A129
  • Orlando, S., Bocchino, F., Miceli, M., Petruk, O., Pumo, M.L., (2012) ApJ, 749, p. 156
  • Petruk, O., Bocchino, F., Miceli, M., (2009) MNRAS, 399, p. 157
  • (2014) A&A, 571, p. A11
  • Rakowski, C.E., Laming, J.M., Hwang, U., (2011) ApJ, 735, p. L21
  • Raymond, J.C., Korreck, K.E., Sedlacek, Q.C., (2007) ApJ, 659, p. 1257
  • Ressler, S.M., Katsuda, S., Reynolds, S.P., (2014) ApJ, 790, p. 85
  • Reynolds, S.P., (2008) ARA&A, 46, p. 89
  • Reynoso, E.M., Hughes, J.P., Moffett, D.A., (2013) AJ, 145, p. 104
  • Rothenflug, R., Ballet, J., Dubner, G., (2004) A&A, 425, p. 121
  • Schure, K.M., Bell, A.R., O'C Drury, L., Bykov, A.M., (2012) Space Sci. Rev., 173, p. 491
  • Uchida, H., Yamaguchi, H., Koyama, K., (2013) ApJ, 771, p. 56
  • Vink, J., (2012) A&ARv, 20, p. 49
  • Winkler, P.F., Gupta, G., Long, K.S., (2003) ApJ, 585, p. 324
  • Winkler, P.F., Williams, B.J., Blair, W.P., (2013) ApJ, 764, p. 156
  • Winkler, P.F., Williams, B.J., Reynolds, S.P., (2014) ApJ, 781, p. 65
  • Xing, Y., Wang, Z., Zhang, X., Chen, Y., (2016) ApJ, 823, p. 44
  • Zirakashvili, V.N., Aharonian, F., (2007) A&A, 465, p. 695

Citas:

---------- APA ----------
Miceli, M., Orlando, S., Pereira, V., Acero, F., Katsuda, S., Decourchelle, A., Winkler, F.P.,..., Dubner, G. (2016) . Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission. Astronomy and Astrophysics, 593.
http://dx.doi.org/10.1051/0004-6361/201628725
---------- CHICAGO ----------
Miceli, M., Orlando, S., Pereira, V., Acero, F., Katsuda, S., Decourchelle, A., et al. "Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission" . Astronomy and Astrophysics 593 (2016).
http://dx.doi.org/10.1051/0004-6361/201628725
---------- MLA ----------
Miceli, M., Orlando, S., Pereira, V., Acero, F., Katsuda, S., Decourchelle, A., et al. "Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission" . Astronomy and Astrophysics, vol. 593, 2016.
http://dx.doi.org/10.1051/0004-6361/201628725
---------- VANCOUVER ----------
Miceli, M., Orlando, S., Pereira, V., Acero, F., Katsuda, S., Decourchelle, A., et al. Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission. Astron. Astrophys. 2016;593.
http://dx.doi.org/10.1051/0004-6361/201628725