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Accurate masses and radii of normal stars: modern results and applications
G Torres, J Andersen, A Giménez - The Astronomy and Astrophysics …, 2010 - Springer
This article presents and discusses a critical compilation of accurate, fundamental
determinations of stellar masses and radii. We have identified 95 detached binary systems …
determinations of stellar masses and radii. We have identified 95 detached binary systems …
[HTML][HTML] Binary stars in the new millennium
Binary stars are as common as single stars. Binary stars are of immense importance to
astrophysicists because that they allow us to determine the masses of the stars independent …
astrophysicists because that they allow us to determine the masses of the stars independent …
batman: basic transit model calculation in Python
L Kreidberg - Publications of the Astronomical Society of the …, 2015 - iopscience.iop.org
I introduce batman, a Python package for modeling exoplanet transit and eclipse light
curves. The batman package supports calculation of light curves for any radially symmetric …
curves. The batman package supports calculation of light curves for any radially symmetric …
exoplanet: Gradient-based probabilistic inference for exoplanet data & other astronomical time series
" exoplanet" is a toolkit for probabilistic modeling of astronomical time series data, with a
focus on observations of exoplanets, using PyMC3 (Salvatier et al., 2016). PyMC3 is a …
focus on observations of exoplanets, using PyMC3 (Salvatier et al., 2016). PyMC3 is a …
A Distance determination to the Small Magellanic Cloud with an accuracy of better than two percent based on late-type eclipsing binary stars
D Graczyk, G Pietrzyński, IB Thompson… - The Astrophysical …, 2020 - iopscience.iop.org
We present a new study of late-type eclipsing binary stars in the Small Magellanic Cloud
(SMC) undertaken with the aim of improving the distance determination to this important …
(SMC) undertaken with the aim of improving the distance determination to this important …
Physics of eclipsing binaries. V. General framework for solving the inverse problem
PHOEBE 2 is a Python package for modeling the observables of eclipsing star systems, but
until now it has focused entirely on the forward model—that is, generating a synthetic model …
until now it has focused entirely on the forward model—that is, generating a synthetic model …
Homogeneous studies of transiting extrasolar planets–IV. Thirty systems with space-based light curves
J Southworth - Monthly Notices of the Royal Astronomical …, 2011 - academic.oup.com
I calculate the physical properties of 32 transiting extrasolar planet and brown-dwarf systems
from existing photometric observations and measured spectroscopic parameters. The …
from existing photometric observations and measured spectroscopic parameters. The …
Detailed models of interacting short-period massive binary stars
Context. The majority of massive stars are part of binary systems. In about a quarter of these,
the companions are so close that mass transfer occurs while they undergo core hydrogen …
the companions are so close that mass transfer occurs while they undergo core hydrogen …
The mass discrepancy in intermediate-and high-mass eclipsing binaries: The need for higher convective core masses
A Tkachenko, K Pavlovski, C Johnston… - Astronomy & …, 2020 - aanda.org
Context. Eclipsing, spectroscopic double-lined binary star systems are excellent laboratories
for calibrating theories of stellar interior structure and evolution. Their precise and accurate …
for calibrating theories of stellar interior structure and evolution. Their precise and accurate …
Homogeneous studies of transiting extrasolar planets–I. Light-curve analyses
J Southworth - Monthly Notices of the Royal Astronomical …, 2008 - academic.oup.com
I present a homogeneous analysis of the transit light curves of 14 well-observed transiting
extrasolar planets. The light curves are modelled using jktebop, random errors are …
extrasolar planets. The light curves are modelled using jktebop, random errors are …