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2018ApJ...852..108F - Astrophys. J., 852, 108-108 (2018/January-2)
A detailed observational analysis of V1324 Sco, the most gamma-ray-luminous classical nova to date.
FINZELL T., CHOMIUK L., METZGER B.D., WALTER F.M., LINFORD J.D., MUKAI K., NELSON T., WESTON J.H.S., ZHENG Y., SOKOLOSKI J.L., MIODUSZEWSKI A., RUPEN M.P., DONG S., STARRFIELD S., CHEUNG C.C., WOODWARD C.E., TAYLOR G.B., BOHLSEN T., BUIL C., PRIETO J., WAGNER R.M., BENSBY T., BOND I.A., SUMI T., BENNETT D.P., ABE F., KOSHIMOTO N., SUZUKI D., TRISTRAM P.J., CHRISTIE G.W., NATUSCH T., McCORMICK J., YEE J. and GOULD A.
Abstract (from CDS):
Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.
Journal keyword(s): gamma rays: stars - novae, cataclysmic variables - radio continuum: stars - stars: individual: V1324 Sco - stars: individual: V1324 Sco
VizieR on-line data: <Available at CDS (J/ApJ/852/108): table1.dat table2.dat table3.dat>
Errata: erratum vol. 903, art. 153 (2020)
Simbad objects: 34
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