The case for jets in cataclysmic variables
DL Coppejans, C Knigge - New Astronomy Reviews, 2020 - Elsevier
For decades cataclysmic variables (CVs) were thought to be one of the few classes of
accreting compact objects to not launch jets, and have consequently been used to constrain …
accreting compact objects to not launch jets, and have consequently been used to constrain …
The ultracompact nature of the black hole candidate X-ray binary 47 Tuc X9
A Bahramian, CO Heinke, V Tudor… - Monthly Notices of …, 2017 - academic.oup.com
Abstract 47 Tuc X9 is a low-mass X-ray binary (LMXB) in the globular cluster 47 Tucanae,
and was previously thought to be a cataclysmic variable. However, Miller-Jones et al …
and was previously thought to be a cataclysmic variable. However, Miller-Jones et al …
Minute-cadence observations of the LAMOST fields with the TMTS: II. Catalogues of short-period variable stars from the first 2-yr surveys
J Lin, X Wang, J Mo, G **, AV Filippenko… - Monthly Notices of …, 2023 - academic.oup.com
Over the past few years, wide-field time-domain surveys such as Zwicky Transient Facility
and Optical Gravitational Lensing Experiment have led to discoveries of various types of …
and Optical Gravitational Lensing Experiment have led to discoveries of various types of …
Cataclysmic Variables from Sloan Digital Sky Survey–V. The search for period bouncers continues
K Inight, BT Gänsicke, A Schwope… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT SDSS-V is carrying out a dedicated survey for white dwarfs, single, and in
binaries, and we report the analysis of the spectroscopy of 118 cataclysmic variables (CVs) …
binaries, and we report the analysis of the spectroscopy of 118 cataclysmic variables (CVs) …
Galactic Model Parameters and Spatial Density of Cataclysmic Variables in the Gaia Era: New Constraints on Population Models
The spatial distribution, Galactic model parameters, and luminosity function of cataclysmic
variables (CVs) are established using reestimated trigonometric parallaxes from Gaia DR3 …
variables (CVs) are established using reestimated trigonometric parallaxes from Gaia DR3 …
1RXH J082623. 6–505741: A New Long-period Cataclysmic Variable with an Evolved Donor and a Low Mass-transfer Rate
KV Sokolovsky, J Strader, SJ Swihart… - The Astrophysical …, 2022 - iopscience.iop.org
We report the discovery of 1RXH J082623. 6− 505741, a 10.4 hr orbital period compact
binary. Modeling extensive optical photometry and spectroscopy reveals a∼ 0.4 M⊙ K-type …
binary. Modeling extensive optical photometry and spectroscopy reveals a∼ 0.4 M⊙ K-type …
SRG/ART-XC Galactic Bulge deep survey. II. Catalogue of point sources
A Semena, I Mereminskiy, A Lutovinov… - Monthly Notices of …, 2024 - academic.oup.com
We present a catalogue of point sources detected with the Mikhail Pavlinsky ART-XC
telescope onboard the SRG observatory during a wide-field survey of the Galactic Bulge that …
telescope onboard the SRG observatory during a wide-field survey of the Galactic Bulge that …
Accretion flows in nonmagnetic white dwarf binaries as observed in X-rays
Ş Balman - Advances in Space Research, 2020 - Elsevier
Abstract Cataclysmic Variables (CVs) are compact binaries with white dwarf (WD) primaries.
CVs and other accreting WD binaries (AWBs) are useful laboratories for studying accretion …
CVs and other accreting WD binaries (AWBs) are useful laboratories for studying accretion …
Classical Novae Masquerading as Dwarf Novae? Outburst Properties of Cataclysmic Variables with ASAS-SN
The unprecedented sky coverage and observing cadence of the All-Sky Automated Survey
for SuperNovae (ASAS-SN) has resulted in the discovery and continued monitoring of a …
for SuperNovae (ASAS-SN) has resulted in the discovery and continued monitoring of a …
Survey of period variations of superhumps in SU UMa-type dwarf novae. IX. The ninth year (2016–2017)
T Kato, K Isogai, FJ Hambsch… - Publications of the …, 2017 - academic.oup.com
Continuing the project described by Kato et al.(, PASJ, 61, S395), we collected times of
superhump maxima for 127 SU UMa-type dwarf novae observed mainly during the 2016 …
superhump maxima for 127 SU UMa-type dwarf novae observed mainly during the 2016 …