Results 121 to 130 of about 86,009 (222)

Series of Dwarf Nova Outbursts in the Post-novae AT Cancri and GK Persei

The Astronomical Journal
AT Cancri and GK Persei are post-novae (Nova Cnc in the seventeenth century and Nova Per 1901). Nowadays, they show episodic brightenings attributed to dwarf nova (DN) outbursts.
Vojtěch Šimon
doaj   +1 more source

Mapping edaphic soils' conditions to identify conservation targets for pine barren and sandplain ecosystems in New York State. [PDF]

Ecol Evol, 2022
Corbin JD, Flatland EL.
europepmc   +1 more source

Fundamental Properties of Novae in M31

The Astrophysical Journal Supplement Series
The peak luminosities and rates of decline for a large sample of novae recently published by Clark et al. have been analyzed using the Yaron et al. nova models to estimate fundamental properties of the M31 nova population.
Allen W. Shafter, Kamil Hornoch
doaj   +1 more source

A Unified Model for Shock Interaction and γ-Ray Emission in Classical Novae

The Astrophysical Journal
We present a parameterized (“toy”) model for shock interaction and γ -ray emission in classical novae, in which a white dwarf envelope of mass M _env is removed over a timescale τ (proportional to the nova speed class, t _2 ) in an outflow that ...
Rebecca Diesing, Brian D. Metzger
doaj   +1 more source

Phosphorus-rich stars with unusual abundances are challenging theoretical predictions. [PDF]

Nat Commun, 2020
Masseron T, García-Hernández DA, Santoveña R, Manchado A, Zamora O, Manteiga M, Dafonte C.   +6 more
europepmc   +1 more source

X-Ray Flashes on Helium Novae

The Astrophysical Journal
A helium nova occurs on a white dwarf (WD) accreting hydrogen-deficient matter from a helium star companion. When the mass of a helium envelope on the WD reaches a critical value, unstable helium burning ignites to trigger a nova outburst.
Mariko Kato, Izumi Hachisu
doaj   +1 more source

Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities. [PDF]

Exp Astron (Dordr), 2021
Rosati P, Basa S, Blain AW, Bozzo E, Branchesi M, Christensen L, Ferrara A, Gomboc A, O'Brien PT, Osborne JP, Rossi A, Schüssler F, Spurio M, Stergioulas N, Stratta G, Amati L, Casewell S, Ciolfi R, Ghirlanda G, Grimm S, Guetta D, Harms J, Le Floc'h E, Longo F, Maggiore M, Mereghetti S, Oganesyan G, Salvaterra R, Tanvir NR, Turriziani S, Vergani SD, Balman S, Caruana J, Erkut MH, Guidorzi G, Frontera F, Martin-Carrillo A, Paltani S, Porquet D, Sergijenko O.   +39 more
europepmc   +1 more source

Unidentified Extremely Red Objects in the field of some Dwarf Novae

, 2003
We present the photometric data of unknown objects discovered in the field of some Dwarf Novae. These objects show extremely red colours: V-Ic > 4 and Rc-H > 5, therefore can be formally classified as EROs.
C. Spogli, M. Fiorucci, G. Nucciarelli, TOSTI, Gino, G. Raimondo   +4 more
core  

Recent progress in understanding the eruptions of classical novae [PDF]

, 1988
Dramatic progress has occurred in the last two decades in understanding the physical processes and events leading up to, and transpiring during the eruption of a classical nova.
Shara, Michael M.
core  

ASASSN-16dv: Superhumps in a Long-period X-Ray-luminous Dwarf Nova

The Astronomical Journal
Combining a long-term light curve, four-color rapid photometry, and spectroscopic and X-ray observations with a 27-day time base TESS light curve, we present the first dedicated study of ASASSN-16dv, detected as a transient in the All-Sky Automated ...
Albert Bruch, Raimundo Lopes de Oliveira, Amanda Silva de Araujo, Romualdo Eleutério, Angela Cristina Krabbe, Koji Mukai   +5 more
doaj   +1 more source