Results 71 to 80 of about 270 (168)

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

open access: yesThe 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   +5 more
doaj   +1 more source

Binary Parameters for the Recurrent Nova T Coronae Borealis

open access: yesThe Astrophysical Journal
T CrB is among the brightest novae. It is recurrent with outbursts happening approximately every 80 yr. The next outburst is imminent, expected in 2025. The T CrB binary consists of an M4 III red giant (RG) secondary and a white dwarf (WD) primary.
Kenneth H. Hinkle   +5 more
doaj   +1 more source

The Long-term Activity of the Postnovae Q Cygni and BK Lyncis

open access: yesThe Astronomical Journal
We show the postnova activity of Q Cyg (Nova Cyg 1876) and BK Lyn (probable Nova Lyn 101). We use both CCD and photographic photometric observations.
Vojtěch Šimon
doaj   +1 more source

The AH Pictoris Syndrome: Continuous Trains of Stunted Outbursts in Novalike Variables

open access: yesThe Astrophysical Journal
Novalike variables are a subgroup of cataclysmic variables (CVs) that—unlike dwarf novae—do not exhibit strong brightenings in their long-term light curves.
Albert Bruch
doaj   +1 more source

Following the Pulsations in the Long-term Cooling of GW Librae and V386 Serpentis

open access: yesThe Astronomical Journal
GW Lib and V386 Ser are dwarf novae systems containing pulsating white dwarfs that underwent large 8–9 mag amplitude outbursts in 2007 and 2019, respectively.
Paula Szkody   +5 more
doaj   +1 more source

Superoutbursts and Positive Superhumps Occurred during the Standstill of a Z Cam-type Dwarf Nova

open access: yesThe Astrophysical Journal
Dwarf novae (DNe) are semidetached binaries, where a white dwarf accretes material from a cool main-sequence companion via an accretion disk, and are known for their intermittent outbursts, making them key systems for studying accretion physics.
Qi-Bin Sun   +6 more
doaj   +1 more source

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

open access: yesNat Commun, 2020
Masseron T   +6 more
europepmc   +1 more source

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

open access: yesExp Astron (Dordr), 2021
Rosati P   +39 more
europepmc   +1 more source

The fungus Kalmusia longispora is able to cause vascular necrosis on Vitis vinifera. [PDF]

open access: yesPLoS One, 2021
Karácsony Z   +4 more
europepmc   +1 more source

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