COLLIMATION AND ASYMMETRY OF THE HOT BLAST WAVE FROM THE RECURRENT NOVA V745 Sco
暂无分享,去创建一个
V. Kashyap | C. Woodward | J. Drake | M. Hernanz | R. Gehrz | J. Ness | K. Page | S. Starrfield | D. V. Rossum | S. Orlando | D. V. van Rossum | J. Laming | L. Delgado
[1] G. Anupama,et al. Insights into the evolution of symbiotic recurrent novae from radio synchrotron emission: V745 Scorpii and RS Ophiuchi , 2015, 1510.02203.
[2] Stony Brook University,et al. Swift detection of the super-swift switch-on of the super-soft phase in nova V745 Sco (2014) , 2015, 1509.04004.
[3] P. Ricker,et al. SIMULATIONS OF THE SYMBIOTIC RECURRENT NOVA V407 CYG. I. ACCRETION AND SHOCK EVOLUTIONS , 2015, 1503.06181.
[4] L. Chomiuk,et al. THE DISTANCE TO NOVA V959 MON FROM VLA IMAGING , 2015, 1503.03899.
[5] J. Drake,et al. X-RAY FADING AND EXPANSION IN THE “MINIATURE SUPERNOVA REMNANT” OF GK PERSEI , 2015, 1503.03181.
[6] F. Harrison,et al. A NuSTAR observation of the fast symbiotic nova V745 Sco in outburst , 2014, 1412.2088.
[7] K. von Braun,et al. The expanding fireball of Nova Delphini 2013 , 2014, Nature.
[8] R. Poleski,et al. Recurrent and symbiotic novae in data from the Optical Gravitational Lensing Experiment , 2014 .
[9] R. Blandford,et al. Fermi Establishes Classical Novae as a Distinct Class of Gamma-ray Sources , 2014 .
[10] J. Guarro,et al. Early evolution of the extraordinary Nova Del 2013 (V339 Del) , 2014, 1407.8212.
[11] L. Chomiuk,et al. The 2011 outburst of recurrent nova T Pyx: X-ray observations expose the white dwarf mass and ejection dynamics , 2014, 1404.3210.
[12] E. Hsiao,et al. NEAR-IR STUDIES OF RECURRENT NOVA V745 SCORPII DURING ITS 2014 OUTBURST , 2014, 1403.0651.
[13] E. Waagen. Nova Sagittarii 2014 = PNV J18250860-2236024 AND Erratum , 2014 .
[14] J. Osborne,et al. Evolving early, hard X-ray emission of V745 Sco , 2014 .
[15] P. Jean,et al. Fermi-LAT Gamma-ray Observations of Recurrent Nova V745 Sco , 2014 .
[16] L. Chomiuk,et al. Detection of Rising Radio Emission from V745 Sco , 2014 .
[17] G. Anupama,et al. Optical observations of the recurrent nova V745 Sco , 2014 .
[18] J. Brooks,et al. HYDROGEN BURNING ON ACCRETING WHITE DWARFS: STABILITY, RECURRENT NOVAE, AND THE POST-NOVA SUPERSOFT PHASE , 2013, 1309.3375.
[19] J. Osborne,et al. Obscuration effects in super-soft-source X-ray spectra , 2013, 1309.2604.
[20] A. Crotts,et al. THE RECURRENT NOVA T Pyx: DISTANCE AND REMNANT GEOMETRY FROM LIGHT ECHOES , 2013, 1305.5245.
[21] H. Mason,et al. CHIANTI—AN ATOMIC DATABASE FOR EMISSION LINES. XIII. SOFT X-RAY IMPROVEMENTS AND OTHER CHANGES , 2013 .
[22] Guillaume Dubus,et al. Particle acceleration and non-thermal emission during the V407 Cygni nova outburst , 2012, 1209.0625.
[23] T. Augusteijn,et al. The spectroscopic evolution of the recurrent nova T Pyxidis during its 2011 outburst. II.The optically thin phase and the structure of the ejecta in recurrent novae , 2012, 1211.3453.
[24] B. Tofflemire,et al. X-RAY GRATING OBSERVATIONS OF RECURRENT NOVA T PYXIDIS DURING THE 2011 OUTBURST , 2012, 1311.2893.
[25] L. Chomiuk,et al. X-RAY EMISSION FROM AN ASYMMETRIC BLAST WAVE AND A MASSIVE WHITE DWARF IN THE GAMMA-RAY EMITTING NOVA V407 Cyg , 2012, 1201.5643.
[26] U. Hwang,et al. A CHANDRA X-RAY SURVEY OF EJECTA IN THE CASSIOPEIA A SUPERNOVA REMNANT , 2011, 1111.7316.
[27] Alan C. Calder,et al. Kelvin–Helmholtz instabilities as the source of inhomogeneous mixing in nova explosions , 2011, Nature.
[28] J. Drake,et al. Modelling the 2010 blast wave of the symbiotic-like nova V407 Cygni , 2011, 1109.5024.
[29] E. Mason. U Scorpii 2010 outburst: observational evidence of an underlying ONeMg white dwarf , 2011, 1107.4013.
[30] J. Dubau,et al. He-like Ions as Practical Astrophysical Plasma Diagnostics: From Stellar Coronae to Active Galactic Nuclei , 2010, 1101.3184.
[31] T Glanzman,et al. Gamma-ray emission concurrent with the nova in the symbiotic binary V407 Cygni. , 2010, Science.
[32] J. J. Drake,et al. THE EARLY BLAST WAVE OF THE 2010 EXPLOSION OF U SCORPII , 2010, 1007.2810.
[33] Max-Planck-Institut fur Radioastronomie,et al. THE EXPANDING NEBULAR REMNANT OF THE RECURRENT NOVA RS OPHIUCHI (2006). II. MODELING OF COMBINED HUBBLE SPACE TELESCOPE IMAGING AND GROUND-BASED SPECTROSCOPY , 2009, 0908.2704.
[34] B. Skiff,et al. VizieR Online Data Catalog , 2009 .
[35] M. F. Bode,et al. X-Ray Spectroscopic Diagnosis of a Wind-Collimated Blast Wave and Metal-Rich Ejecta from the 2006 Explosion of RS Ophiuchi , 2009 .
[36] J. J. Drake,et al. Three-dimensional modeling of the asymmetric blast wave from the 2006 outburst of RS Ophiuchi: Early X-ray emission , 2008, 0811.3941.
[37] J. Osborne,et al. HIGH-RESOLUTION X-RAY SPECTROSCOPY OF THE EVOLVING SHOCK IN THE 2006 OUTBURST OF RS OPHIUCHI , 2008, 0810.2023.
[38] Michael P. Rupen,et al. Uncovering the Nature of Nova Jets: A Radio Image of Highly Collimated Outflows from RS Ophiuchi , 2008 .
[39] Rolf Walder,et al. 3D simulations of RS Ophiuchi : from accretion to nova blast , 2008, 0804.2628.
[40] M. Rupen,et al. An Expanding Shell and Synchrotron Jet in RS Ophiuchi , 2007, 0711.1142.
[41] Marina Orio,et al. X-Ray Spectroscopy of the 2006 Outburst of RS Ophiuchi , 2007, 0709.4512.
[42] Matthew W. Muterspaugh,et al. Interferometric Observations of V1663 Aquilae (Nova Aql 2005) , 2007 .
[43] Space Telescope Sceince Institute,et al. Hubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of the Recurrent Nova RS Ophiuchi , 2007, 0706.2745.
[44] M. Hernanz,et al. Evidence for Nonlinear Diffusive Shock Acceleration of Cosmic Rays in the 2006 Outburst of the Recurrent Nova RS Ophiuchi , 2007, 0705.4422.
[45] L. Bildsten,et al. Thermally Stable Nuclear Burning on Accreting White Dwarfs , 2007, astro-ph/0702049.
[46] R. Davis,et al. An asymmetric shock wave in the 2006 outburst of the recurrent nova RS Ophiuchi , 2006, Nature.
[47] N. Gehrels,et al. Swift Observations of the 2006 Outburst of the Recurrent Nova RS Ophiuchi. I. Early X-Ray Emission from the Shocked Ejecta and Red Giant Wind , 2006, astro-ph/0604618.
[48] K. Nomoto,et al. Thermal Stability of White Dwarfs Accreting Hydrogen-rich Matter and Progenitors of Type Ia Supernovae , 2006, astro-ph/0603351.
[49] L. Althaus,et al. Mass-radius relations for massive white dwarf stars , 2005, astro-ph/0507559.
[50] Peter W. A. Roming,et al. The Swift Ultra-Violet/Optical Telescope , 2002, SPIE Optics + Photonics.
[51] D. Dewey,et al. An Overview of the Performance of the Chandra X-ray Observatory , 2003, astro-ph/0503319.
[52] U. Hwang,et al. On the Determination of Ejecta Structure and Explosion Asymmetry from the X-Ray Knots of Cassiopeia A , 2003, astro-ph/0306119.
[53] H. Duerbeck,et al. The CTIO nova survey: data , 2003 .
[54] M. Bode,et al. Echoes of an Explosive Past: Solving the Mystery of the First Superluminal Source , 2003 .
[55] D. Dewey,et al. High-Resolution X-Ray Spectra of Capella: Initial Results from the Chandra High-Energy Transmission Grating Spectrometer , 2000, astro-ph/0006457.
[56] Heinrich W. Braeuninger,et al. Description and performance of the low-energy transmission grating spectrometer on board Chandra , 2000, Astronomical Telescopes and Instrumentation.
[57] Mariko Kato,et al. Optically thick wind solutions for an extremely rapid light curve of recurrent novae , 1999 .
[58] J. Truran,et al. Evolutionary sequences for Nova V1974 Cygni using new nuclear reaction rates and opacities , 1998 .
[59] C. Done,et al. Complex absorption and reflection of a multitemperature cyclotron–bremsstrahlung X-ray cooling shock in BY Cam , 1997, astro-ph/9712226.
[60] H. Mason,et al. CHIANTI - an atomic database for emission lines - I. Wavelengths greater than 50 Å , 1997 .
[61] Mario Livio,et al. On the interpretation and implications of nova abundances: An abundance of riches or an overabundance of enrichments , 1994 .
[62] J. J. Johnson,et al. Infrared observations of the recurrent novae V745 Sco and V3890 Sgr , 1993 .
[63] A. King,et al. Iron Kα lines and the absorption structure of intermediate polars , 1991 .
[64] L. Stella,et al. Iron Line Diagnostics in X-ray Sources , 1991 .
[65] H. Duerbeck. V745 Sco - a new member of the elusive group of recurrent novae. , 1989 .
[66] A. Taylor,et al. VLBI observations of RS Oph – a recurrent nova with non-spherical ejection , 1989 .
[67] N. Grevesse,et al. Abundances of the elements: Meteoritic and solar , 1989 .
[68] Warren M. Sparks,et al. A model for the 1987 outburst of the recurrent Nova U Scorphii , 1988 .
[69] M. Reid,et al. The distance to the center of the Galaxy , 1987 .
[70] J. W. Truran,et al. On the frequency of occurrence of oxygen-neon-magnesium white dwarfs in classical nova systems , 1986 .
[71] A. R. Taylor,et al. Radio observations of the 1985 outburst of RS Ophiuchi , 1986 .
[72] N. Gehrels. Confidence limits for small numbers of events in astrophysical data , 1986 .
[73] M. F. Bode,et al. A model for the outburst of nova RS Ophiuchi in 1985 , 1985 .
[74] Mariko Kato,et al. Optically thick winds and nova outbursts , 1994 .
[75] B. Fryxell,et al. Finite propagation time in multidimensional thermonuclear runaways , 1982 .
[76] M. Fujimoto. A theory of hydrogen shell flashes on accreting white dwarfs. I - Their progress and the expansion of the envelope. II - The stable shell burning and the recurrence period of shell flashes , 1982 .
[77] D. Sugimoto. Symposium on Fundamental Problems in the Theory of Stellar Evolution , 1981 .
[78] W. Cash,et al. Parameter estimation in astronomy through application of the likelihood ratio. [satellite data analysis techniques , 1979 .
[79] J. Truran,et al. CNO abundances and hydrodynamic models of the nova outburst. III - 0.5 solar mass models with enhanced carbon, oxygen, and nitrogen , 1974 .
[80] J. Hutchings. The Non-Spherical Nebulae of Nova Delphini 1967, Nova Vulpeculae 1968(1), and Nova Serpentis 1970 , 1972 .
[81] A. H. Gabriel,et al. Interpretation of Solar Helium-Like Ion Line Intensities , 1969 .
[82] J. Cole,et al. Similarity and Dimensional Methods in Mechanics , 1960 .