CARBON MONOXIDE IN THE COLD DEBRIS OF SUPERNOVA 1987A
暂无分享,去创建一个
R. Kirshner | R. McCray | J. Kamenetzky | A. Bolatto | R. Indebetouw | M. Barlow | J. Blommaert | A. Soderberg | B. Swinyard | L. Decin | M. Baes | G. Zanardo | L. Dunne | I. Martí-Vidal | M. Groenewegen | M. Matsuura | G. Sonneborn | C. Fransson | L. Staveley-Smith | J. Glenn | H. Gomez | J. Yates | R. Hopwood | P. Royer | J. V. van Loon | M. Meixner | P. V. van Hoof | J. Marcaide | G. Van de Steene | M. Lakicevic | G. C. Van de Steene
[1] A. Tzioumis,et al. HIGH-RESOLUTION RADIO OBSERVATIONS OF THE REMNANT OF SN 1987A AT HIGH FREQUENCIES , 2013, 1301.6527.
[2] J. Sollerman,et al. THE MORPHOLOGY OF THE EJECTA IN SUPERNOVA 1987A: A STUDY OVER TIME AND WAVELENGTH , 2012, 1212.5051.
[3] J. Sollerman,et al. LATE SPECTRAL EVOLUTION OF THE EJECTA AND REVERSE SHOCK IN SN 1987A , 2012, 1212.5052.
[4] G. Zanardo,et al. The remnant of supernova 1987A resolved at 3-mm wavelength , 2012, 1203.4982.
[5] J. Rho,et al. SPECTROSCOPIC DETECTION OF CARBON MONOXIDE IN THE YOUNG SUPERNOVA REMNANT CASSIOPEIA A , 2012, 1202.4540.
[6] M. Sauvage,et al. Herschel Detects a Massive Dust Reservoir in Supernova 1987A , 2011, Science.
[7] G. Zanardo,et al. The remnant of SN 1987A revealed at (sub-)mm wavelengths , 2011, 1107.1323.
[8] A. Sarangi,et al. Molecules in Supernova Ejecta , 2011, Proceedings of the International Astronomical Union.
[9] C. Fransson,et al. The 44Ti-powered spectrum of SN 1987A , 2011, 1103.3653.
[10] O. Krause,et al. MESS (Mass-loss of Evolved StarS), a Herschel key program , 2010, 1012.2701.
[11] William T. Reach,et al. THE THREE-DIMENSIONAL STRUCTURE OF CASSIOPEIA A , 2010, 1011.3858.
[12] William T. Reach,et al. THE THREE-DIMENSIONAL STRUCTURE OF INTERIOR EJECTA IN CASSIOPEIA A AT HIGH SPECTRAL RESOLUTION , 2010, 1006.0918.
[13] S. Ott,et al. Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy , 2010, 1005.5331.
[14] S. J. Liu,et al. Herschel : the first science highlights Special feature L etter to the E ditor The Herschel-SPIRE instrument and its in-flight performance , 2010 .
[15] R. C. Forrey,et al. ROTATIONAL QUENCHING OF CO DUE TO H2 COLLISIONS , 2010, 1004.3923.
[16] B. Leibundgut,et al. The 3-D structure of SN 1987A's inner ejecta , 2010, 1003.5684.
[17] E. Dwek,et al. THE CHEMISTRY OF POPULATION III SUPERNOVA EJECTA. I. FORMATION OF MOLECULES IN THE EARLY UNIVERSE , 2009, 0907.3621.
[18] Doug Henke,et al. Optics Design and Verification for the APEX Swedish Heterodyne Facility Instrument (SHeFI) , 2009 .
[19] A. Tzioumis,et al. Fourier Modeling of the Radio Torus Surrounding SN 1987A , 2008, 0805.4195.
[20] R. McCray,et al. Supernova 1987A at Age 20 , 2007 .
[21] K. Cooper. Supernova 1987A - 20 years on , 2007 .
[22] R. McCray,et al. Supernova 1987A : 20 years after : Supernovae and Gamma-Ray Bursters : Aspen, Colorado, 19-23 February 2007 , 2007 .
[23] N. Balakrishnan,et al. Quantum-Mechanical Study of Rotational and Vibrational Transitions in CO Induced by H Atoms , 2002 .
[24] J. Beaulieu,et al. NEW VIEWS OF THE MAGELLANIC CLOUDS , 1999 .
[25] A. Dalgarno,et al. The Oxygen Temperature of SN 1987A , 1995 .
[26] S. Green. Collisional excitation of CO by H2O - An astrophysicist's guide to obtaining rate constants from coherent anti-Stokes Raman line shape data , 1993 .
[27] R. McCray. Supernova 1987A Revisited , 1993 .
[28] A. Dalgarno,et al. Carbon Monoxide in SN 1987A , 1992 .
[29] R. Kirshner,et al. Properties of the SN 1987A Circumstellar Ring and the Distance to the Large Magellanic Cloud , 1991 .
[30] S. Woosley. SN 1987A: After the Peak , 1988 .
[31] J. Castor. Spectral line formation in Wolf-Rayet envelopes. , 1970 .