Magnetic fields of M dwarfs
O Kochukhov - The Astronomy and Astrophysics Review, 2021 - Springer
Magnetic fields play a fundamental role for interior and atmospheric properties of M dwarfs
and greatly influence terrestrial planets orbiting in the habitable zones of these low-mass …
and greatly influence terrestrial planets orbiting in the habitable zones of these low-mass …
Stellar multiplicity
Stellar multiplicity is a ubiquitous outcome of the star-formation process. The frequency and
main characteristics of multiple systems, and their dependence on primary mass and …
main characteristics of multiple systems, and their dependence on primary mass and …
CARMENES input catalogue of M dwarfs-V. Luminosities, colours, and spectral energy distributions
C Cifuentes, JA Caballero, M Cortés-Contreras… - Astronomy & …, 2020 - aanda.org
Context. The relevance of M dwarfs in the search for potentially habitable Earth-sized
planets has grown significantly in the last years. Aims. In our on-going effort to …
planets has grown significantly in the last years. Aims. In our on-going effort to …
The Transiting Exoplanet Survey Satellite: simulations of planet detections and astrophysical false positives
PW Sullivan, JN Winn… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT The Transiting Exoplanet Survey Satellite (TESS) is a NASA-sponsored
Explorer mission that will perform a wide-field survey for planets that transit bright host stars …
Explorer mission that will perform a wide-field survey for planets that transit bright host stars …
Kepler flares. I. Active and inactive M dwarfs
SL Hawley, JRA Davenport, AF Kowalski… - The Astrophysical …, 2014 - iopscience.iop.org
We analyzed Kepler short-cadence M dwarf observations. Spectra from the Astrophysical
Research Consortium 3.5 m telescope identify magnetically active (Hα in emission) stars …
Research Consortium 3.5 m telescope identify magnetically active (Hα in emission) stars …
The big problems in star formation: the star formation rate, stellar clustering, and the initial mass function
MR Krumholz - Physics Reports, 2014 - Elsevier
Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …
generation of radiant energy, synthesis of elements, formation of planets, and development …
Kepler planet occurrence rates for mid-type M dwarfs as a function of spectral type
KK Hardegree-Ullman, MC Cushing… - The Astronomical …, 2019 - iopscience.iop.org
Previous studies of planet occurrence rates largely relied on photometric stellar
characterizations. In this paper, we present planet occurrence rates for mid-type M dwarfs …
characterizations. In this paper, we present planet occurrence rates for mid-type M dwarfs …
The 10 parsec sample in the Gaia era
C Reylé, K Jardine, P Fouqué, JA Caballero… - Astronomy & …, 2021 - aanda.org
Context. The nearest stars provide a fundamental constraint for our understanding of stellar
physics and the Galaxy. The nearby sample serves as an anchor where all objects can be …
physics and the Galaxy. The nearby sample serves as an anchor where all objects can be …
Stars, gas, and dark matter in the solar neighborhood
CF McKee, A Parravano… - The Astrophysical …, 2015 - iopscience.iop.org
STARS, GAS, AND DARK MATTER IN THE SOLAR NEIGHBORHOOD - IOPscience This
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site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
[PDF][PDF] The stellar and sub-stellar IMF of simple and composite populations
P Kroupa, C Weidner, J Pflamm-Altenburg… - arXiv preprint arXiv …, 2011 - Citeseer
The current knowledge on the stellar IMF is documented. It is usually described as being
invariant, but evidence to the contrary has emerged: it appears to become top-heavy when …
invariant, but evidence to the contrary has emerged: it appears to become top-heavy when …