Abundance Analysis of the Extremely Fast ONeMg Novae V838 Herculis and V4160 Sagittarii
暂无分享,去创建一个
Steven N. Shore | Sumner Starrfield | Greg J. Schwarz | S. Starrfield | G. Schwarz | S. Shore | K. Vanlandingham | Karen Michelle Vanlandingham
[1] S. Bowyer,et al. Extreme Ultraviolet Astronomy , 1991 .
[2] J. Truran,et al. A prediction of the gamma-ray flux from Nova Herculis 1991 , 1992 .
[3] Michel Casse,et al. Origin and evolution of the elements , 1993 .
[4] Mario Livio,et al. The Calibration of Novae as Distance Indicators , 1995 .
[5] New Elemental Abundances for V1974 Cygni , 2005, astro-ph/0501648.
[6] D. Harman,et al. Hubble Space Telescope imaging and ground-based spectroscopy of old nova shells — II. The bipolar shell of the slow nova HR Del , 2003 .
[7] P. Szkody,et al. PHOTOMETRY AND SPECTROSCOPY OF NOVA HERCULIS 1991 , 1992 .
[8] P. Hauschildt,et al. Spatially Resolved Spectra of V1974 Cygni (Nova Cygni 1992) with the Goddard High Resolution Spectrograph , 1997 .
[9] George Sonneborn,et al. Optical and ultraviolet spectrophotometry of the ONeMg Nova V838 Herculis 1991 , 1996 .
[10] J. Krautter,et al. The Early Ultraviolet Evolution of the ONeMg Nova V382 Velorum 1999 , 2003, astro-ph/0301415.
[11] Roberto Gilmozzi,et al. HST Imagery of the Non-Expanding, Clumped "Shell" of the Recurrent Nova T Pyxidis , 1997 .
[12] O. Yaron,et al. An Extended Grid of Nova Models. II. The Parameter Space of Nova Outbursts , 2005 .
[13] Steven N. Shore,et al. The Ultraviolet and X-ray View of the Demise of Nova V1974 Cygni , 1996 .
[14] M. F. Bode,et al. AN INTERACTING WINDS MODEL FOR THE X-RAY-EMISSION FROM V838 HER (NOVA-HERCULIS 1991) , 1994 .
[15] ROBERT E. Williams,et al. The Formation of Novae Spectra , 1992 .
[16] Steven N. Shore,et al. Nuclear Turnoff Times for ONeMg Novae Determined Using Ultraviolet Spectral Evolution , 2001 .
[17] J. Truran,et al. Hydrodynamic Studies of Accretion onto Massive White Dwarfs: ONeMg-enriched Nova Outbursts , 1995 .
[18] D. Prialnik,et al. An extended grid of multicycle nova evolution models , 1995 .
[19] M. F. Bode,et al. X-ray detection of Nova Herculis 1991 five days after optical outburst , 1992, Nature.
[20] J. Truran,et al. The Effects of New Nuclear Reaction Rates and Opacities on Hydrodynamic Simulations of the Nova Outburst , 2000 .
[21] D. Schlegel,et al. Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.
[22] J. José,et al. Synthesis of Intermediate-Mass Elements in Classical Novae: From Si to Ca , 2001, astro-ph/0106418.
[23] J. Hackwell,et al. 8-13 micron spectroscopy of Nova Herculis 1991 , 1992 .
[24] S. Starrfield,et al. Elemental abundances for Nova V693 Coronae Austrinae 1981 , 1997 .
[25] J. Miles,et al. The Mid-Infrared Evolution of Nova V1974 Cygni , 1996 .
[26] G. Schwarz. A New Abundance Analysis of the ONeMg Nova QU Vulpeculae , 2002 .
[27] G. Ferland,et al. CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra , 1998 .
[28] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[29] Robert D. Gehrz,et al. The peculiar, fast Nova Herculis 1991 , 1992 .
[30] J. José,et al. Nucleosynthesis in Classical Novae: CO versus ONe White Dwarfs , 1997, astro-ph/9709153.
[31] L. Bildsten,et al. Theoretical Modeling of the Thermal State of Accreting White Dwarfs Undergoing Classical Nova Cycles , 2004 .
[32] L. Ho,et al. Nova Herculis 1991 : thermonuclear runaway on a massive ONeMg white dwarf , 1993 .
[33] M. M. Phillips,et al. The Tololo nova survey: Spectra of recent novae , 1994 .