Classical novae, explosions that result from thermonuclear runaways (TNRs) on the
surfaces of white dwarfs (WDs) accreting hydrogen‐rich matter in close binary systems, are …

An optical imaging study of 30 recent novae has been undertaken using both ground-based
and space-based observations. Resolved shells have been detected around nine objects in …

The outburst of Nova V1974 Cyg 1992 is arguably the best observed of this century, with
realistic estimates now available for the amount of mass ejected, the composition of the …

We calculate many different nova light curves for a variety of white dwarf masses and
chemical compositions, with the assumption that free-free emission from optically thin ejecta …

The nova outburst is a consequence of the accretion of hydrogen-rich material onto a white
dwarf in a close binary system and observations show that the accreting material must have …

Aims. Among the classical novae, the ONe subgroup, distinguished by their large
overabundance of neon, are thought to occur on the most massive white dwarfs. Nova Mon …

ABSTRACT V392 Persei is a known dwarf nova (DN) that underwent a classical nova
eruption in 2018. Here we report ground-based optical, Swift UV and X-ray, and Fermi-LAT γ …

The Swift gamma-ray burst satellite is an excellent facility for studying novae. Its rapid
response time and sensitive X-ray detector provides an unparalleled opportunity to …

We analyzed light curves of five neon novae, QU Vul, V351 Pup, V382 Vel, V693 CrA, and
V1974 Cyg, and determined their white dwarf (WD) masses and distance moduli on the …

We present an analysis of optical and UV spectra of the fast nova V838 Herculis 1991. IUE
observations began on 1991 March 25 and continued through 1991 August 20, while optical …