Circumbinary accretion: From binary stars to massive binary black holes
We review recent works on the dynamics of circumbinary accretion, including time variability,
angular momentum transfer between the disk and the binary, and the secular evolution of …
angular momentum transfer between the disk and the binary, and the secular evolution of …
Microlensing searches for exoplanets
Y Tsapras - Geosciences, 2018 - mdpi.com
Gravitational microlensing finds planets through their gravitational influence on the light
coming from a more distant background star. The presence of the planet is then inferred from …
coming from a more distant background star. The presence of the planet is then inferred from …
A Jovian analogue orbiting a white dwarf star
Studies, have shown that the remnants of destroyed planets and debris-disk planetesimals
can survive the volatile evolution of their host stars into white dwarfs,, but few intact planetary …
can survive the volatile evolution of their host stars into white dwarfs,, but few intact planetary …
Predictions of the WFIRST microlensing survey. I. Bound planet detection rates
Abstract The Wide Field InfraRed Survey Telescope (WFIRST) is the next NASA
astrophysics flagship mission, to follow the James Webb Space Telescope. The WFIRST …
astrophysics flagship mission, to follow the James Webb Space Telescope. The WFIRST …
The exoplanet mass-ratio function from the MOA-II survey: discovery of a break and likely peak at a neptune mass
D Suzuki, DP Bennett, T Sumi, IA Bond… - The Astrophysical …, 2016 - iopscience.iop.org
We report the results of the statistical analysis of planetary signals discovered in MOA-II
microlensing survey alert system events from 2007 to 2012. We determine the survey …
microlensing survey alert system events from 2007 to 2012. We determine the survey …
The degree of alignment between circumbinary disks and their binary hosts
All four circumbinary (CB) protoplanetary disks orbiting short-period (P< 20 days) double-
lined spectroscopic binaries (SB2s)—a group that includes UZ Tau E, for which we present …
lined spectroscopic binaries (SB2s)—a group that includes UZ Tau E, for which we present …
Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet
W Zang, KH Hwang, A Udalski, T Wang… - The Astronomical …, 2021 - iopscience.iop.org
In order to exhume the buried signatures of" missing planetary caustics" in Korea
Microlensing Telescope Network (KMTNet) data, we conducted a systematic anomaly …
Microlensing Telescope Network (KMTNet) data, we conducted a systematic anomaly …
WFIRST Exoplanet Mass-measurement Method Finds a Planetary Mass of 39±8 M⊕ for OGLE-2012-BLG-0950Lb
A Bhattacharya, JP Beaulieu, DP Bennett… - The Astronomical …, 2018 - iopscience.iop.org
WFIRST Exoplanet Mass-measurement Method Finds a Planetary Mass of 39 ± 8 M⊕ for
OGLE-2012-BLG-0950Lb - IOPscience This site uses cookies. By continuing to use this site you …
OGLE-2012-BLG-0950Lb - IOPscience This site uses cookies. By continuing to use this site you …
BEBOP III. Observations and an independent mass measurement of Kepler-16 (AB) b–the first circumbinary planet detected with radial velocities
AHMJ Triaud, MR Standing, N Heidari… - Monthly Notices of …, 2022 - academic.oup.com
The radial velocity method is amongst the most robust and most established means of
detecting exoplanets. Yet, it has so far failed to detect circumbinary planets despite their …
detecting exoplanets. Yet, it has so far failed to detect circumbinary planets despite their …
Demographics of Exoplanets in Binaries. I. Architecture of S-type Planetary Systems Revealed by the Radial-velocity Sample
XN Su, JW Xie, JL Zhou, P Thebault - The Astronomical Journal, 2021 - iopscience.iop.org
Although the sample of exoplanets in binaries has been greatly expanded, the sample
heterogeneity and observational bias are obstacles toward a clear figure of exoplanet …
heterogeneity and observational bias are obstacles toward a clear figure of exoplanet …