Beryllium detection in the very fast nova ASASSN-16kt (V407 Lupi)

LI, CT, ZC and AdUP acknowledge support from the Spanish research project AYA 2014-58381-P. CT and AdUP furthermore acknowledge support from Ramn y Cajal fellowships Ramon y Cajal (RyC)-2012-09984 and RyC-2012-09975. ZC also acknowledges support from the Juan de la Cierva Incorporacion fellowship IJCI-2014-21669. LV acknowledge support from Commission Nacional de Investigacion Cientifica y Tecnologica (CONICYT) through project Fondecyt n. 1171364. AZ acknowledge support from Conicyt through the 'Beca Doctorado Nacional' 21170536. Support for JLP is provided in part by Fondo Nacional de Desarrollo Cientifico y Tecnologico (FONDECYT) through the grant 1151445 and by the Ministry of Economy, Development, and Tourism's Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS.

[1]  Astrophysics,et al.  The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0 , 2017, 1706.07060.

[2]  M. Valle,et al.  Highly enriched 7Be in the ejecta of Nova Sagittarii 2015 No. 2 (V5668 Sgr) and the Galactic 7Li origin , 2016, 1609.07297.

[3]  Rafael Brahm,et al.  CERES: A Set of Automated Routines for Echelle Spectra , 2016, 1609.02279.

[4]  A. Arai,et al.  THE 7Be ii RESONANCE LINES IN TWO CLASSICAL NOVAE V5668 SGR AND V2944 OPH , 2016, 1601.05168.

[5]  S. Cristallo,et al.  Do we really know Mup (i.e. the transition mass between Type Ia and core-collapse supernova progenitors)? , 2016 .

[6]  Z. Gácsi,et al.  Observation of Anomalous Internal Pair Creation in ^{8}Be: A Possible Indication of a Light, Neutral Boson. , 2015, Physical review letters.

[7]  L. Pasquini,et al.  EARLY OPTICAL SPECTRA OF NOVA V1369 CEN SHOW THE PRESENCE OF LITHIUM , 2015, 1506.08048.

[8]  V. Dhillon,et al.  Searching for nova shells around cataclysmic variables , 2015, 1505.06048.

[9]  Akira Arai,et al.  Explosive lithium production in the classical nova V339 Del (Nova Delphini 2013) , 2015, Nature.

[10]  Koji Mukai,et al.  Binary orbits as the driver of γ-ray emission and mass ejection in classical novae , 2014, Nature.

[11]  W. Freudling,et al.  Automated data reduction workflows for astronomy , 2013, 1311.5411.

[12]  J. Prieto,et al.  THE MAN BEHIND THE CURTAIN: X-RAYS DRIVE THE UV THROUGH NIR VARIABILITY IN THE 2013 ACTIVE GALACTIC NUCLEUS OUTBURST IN NGC 2617 , 2013, 1310.2241.

[13]  Prasanth H. Nair,et al.  Astropy: A community Python package for astronomy , 2013, 1307.6212.

[14]  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.

[15]  S. Shore Spectroscopy of Novae - A User's Manual , 2012, 1211.3176.

[16]  Carlos Guirao,et al.  PUCHEROS: a cost-effective solution for high-resolution spectroscopy with small telescopes , 2012 .

[17]  M. F. Bode,et al.  The expanding dusty bipolar nebula around the nova V1280 Scorpi , 2012, 1207.5301.

[18]  Gaël Varoquaux,et al.  The NumPy Array: A Structure for Efficient Numerical Computation , 2011, Computing in Science & Engineering.

[19]  E. Ofek,et al.  DISCOVERY OF A NEW PHOTOMETRIC SUB-CLASS OF FAINT AND FAST CLASSICAL NOVAE , 2010, 1003.1720.

[20]  D. York,et al.  STUDIES OF DIFFUSE INTERSTELLAR BANDS V. PAIRWISE CORRELATIONS OF EIGHT STRONG DIBs AND NEUTRAL HYDROGEN, MOLECULAR HYDROGEN, AND COLOR EXCESS , 2010, 1011.2951.

[21]  I. Steele,et al.  The morphology of the expanding ejecta of V2491 Cygni (2008 N.2) , 2010, 1011.2045.

[22]  F. Timmes,et al.  THE EFFECTS OF THE pep NUCLEAR REACTION AND OTHER IMPROVEMENTS IN THE NUCLEAR REACTION RATE LIBRARY ON SIMULATIONS OF THE CLASSICAL NOVA OUTBURST , 2008, 0811.0197.

[23]  M. Valle,et al.  Transient Heavy Element Absorption Systems in Novae: Episodic Mass Ejection from the Secondary Star , 2008, 0805.1372.

[24]  John D. Hunter,et al.  Matplotlib: A 2D Graphics Environment , 2007, Computing in Science & Engineering.

[25]  S. Sarkar,et al.  Big-Bang Nucleosynthesis , 2014, 1412.1408.

[26]  W. B. Burton,et al.  The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI - Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections , 2005, astro-ph/0504140.

[27]  Astronomy,et al.  An Extended Grid of Nova Models. II. The Parameter Space of Nova Outbursts , 2005, astro-ph/0503143.

[28]  K. Lodders,et al.  The Imprint of Nova Nucleosynthesis in Presolar Grains , 2002, astro-ph/0405332.

[29]  L. Pasquini,et al.  The evolution of Nova V382 Velorum 1999 , 2002, astro-ph/0205135.

[30]  H. Duerbeck,et al.  Optical Imaging of Nova Shells and the Maximum Magnitude-Rate of Decline Relationship , 2000, astro-ph/0006458.

[31]  T. O’brien,et al.  Hubble Space Telescope imaging and ground-based spectroscopy of old nova shells – I. FH Ser, V533 Her, BT Mon, DK Lac and V476 Cyg , 2000, astro-ph/0001092.

[32]  M. Livio,et al.  The Spectroscopic Differences between Disk and Thick-Disk/Bulge Novae , 1998 .

[33]  C. D. GillT.J. O'Brien,et al.  Deep optical imaging of nova remnants: a southern sky sample , 1998, astro-ph/9806076.

[34]  J. Truran,et al.  Evolutionary sequences for Nova V1974 Cygni using new nuclear reaction rates and opacities , 1998 .

[35]  J. José,et al.  Nucleosynthesis in Classical Novae: CO versus ONe White Dwarfs , 1997, astro-ph/9709153.

[36]  R. Gehrz,et al.  Nucleosynthesis in Classical Novae and Its Contribution to the Interstellar Medium , 1998 .

[37]  J. José,et al.  On the Synthesis of 7Li and 7Be in Novae , 1996 .

[38]  Mario Livio,et al.  The Calibration of Novae as Distance Indicators , 1995 .

[39]  J. Dunlop,et al.  A deep optical imaging study of the nebular remnants of classical novae , 1995 .

[40]  R. Shaw,et al.  SOFTWARE FOR THE ANALYSIS OF EMISSION LINE NEBULAE , 1995 .

[41]  Robert E. Williams Extinction, ejecta masses, and radial velocities of novae , 1994 .

[42]  C. Woodward,et al.  The Temporal Evolution of the 4--14 Micron Spectrum of V1974 Cygni (Nova Cygni 1992) , 1994 .

[43]  Sidney van den Bergh THE HUBBLE PARAMETER , 1992 .

[44]  ROBERT E. Williams,et al.  The Formation of Novae Spectra , 1992 .

[45]  M. Livio Classical novae and the extragalactic distance scale , 1992 .

[46]  J. Truran,et al.  Hydrodynamic Studies of Accretion onto Massive White Dwarfs: ONeMg-enriched Nova Outbursts , 1995 .

[47]  M. M. Phillips,et al.  The Evolution and Classification of Postoutburst Novae Spectra , 1991 .

[48]  D. Osterbrock,et al.  Astrophysics of Gaseous Nebulae and Active Galactic Nuclei , 1989 .

[49]  S. Starrfield,et al.  Of Galactic Novae , 1987 .

[50]  J. W. Truran,et al.  On the frequency of occurrence of oxygen-neon-magnesium white dwarfs in classical nova systems , 1986 .

[51]  A. V. Tutukov,et al.  On the evolution of close binaries with components of initial mass between 3 solar masses and 12 solar masses , 1985 .

[52]  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 .

[53]  M. Livio,et al.  On the role of the accretion rate in nova outbursts , 1982 .

[54]  J. Truran,et al.  On Li-7 production in nova explosions , 1978 .

[55]  J. Black,et al.  Oscillator strengths and ground-state photoionization cross-sections for Mg+ and Ca+. , 1972 .

[56]  A. G. W. Cameron,et al.  Lithium and the s-process in red-giant stars , 1971 .

[57]  A. A. Boyarchuk,et al.  Structure of envelopes ejected by Novae , 1970 .

[58]  William A. Fowler,et al.  Thermonuclear Reaction Rates, III , 1967 .

[59]  William A. Fowler,et al.  On the Synthesis of elements at very high temperatures , 1967 .

[60]  Cecilia Payne-Gaposchkin,et al.  The Galactic Novae , 1958 .

[61]  G. Vaucouleurs,et al.  Novae in the Magellanic Clouds and in the Galaxy , 1955 .

[62]  D. B. Mclaughlin Spectral Stages of Novae. , 1942 .

[63]  K. Schwarzschild,et al.  The Observatory , 1886 .