Results 81 to 90 of about 23,116,162 (197)
The chemical abundances of stars in galaxies are a fossil record of the star formation and stellar evolution processes that regulate galaxy formation, including the stellar initial mass function, the fraction and timing of type Ia supernovae (SNeIa), and
Andersson Eric P. +8 more
doaj +1 more source
The SDSS White Dwarf - M Star Library
to appear in the ASP Conference Series on "Evolution of Compact Binaries" (ESO), Vi\~na del Mar ...
Heller, René +2 more
openaire +2 more sources
Study determined if 2MASS photometric data are reliable for luminosity classification using JHK plots of Reid and Hawley (2001). Effects of interstellar reddening on the placement of giant and dwarf data on the JIIK plot were analyzed. Dwarfs (N=54) were
Furiak, Nicolas M.
core
On the Possibility of an Upper Limit on Magnetically Induced Radius Inflation in Low-mass Stars
The radii of low-mass stars are observed to be inflated above standard model predictions, especially in magnetically active stars. Typically, the empirical relative radius inflations Δ R / R are ≤10% but in (rare) cases may be ≥20%.
J. MacDonald, D. J. Mullan
doaj +1 more source
Transiting Jupiters around M Dwarfs Have Similar Masses to FGK Warm Jupiters
This paper presents a comparative analysis of the bulk properties (mass and radius) of transiting giant planets (≳8 R _⊕ ) orbiting FGKM stars. Our findings suggest that the average mass of M-dwarf Jupiters is lower than that of their solar-type ...
Shubham Kanodia
doaj +1 more source
Habitable Zone Lifetime of Exoplanets around Main Sequence Stars [PDF]
Funding: Dean's Scholarship at the University of East Anglia.The potential habitability of newly discovered exoplanets is initially assessed by determining whether their orbits fall within the circumstellar habitable zone of their star.
Claire, M. +3 more
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JWST/NIRCam Detection of the Fomalhaut C Debris Disk in Scattered Light
Observations of debris disks offer important insights into the formation and evolution of planetary systems. Though M dwarfs make up approximately 80% of nearby stars, very few M dwarf debris disks have been studied in detail—making it unclear how or if ...
Kellen Lawson +22 more
doaj +1 more source
Confirmation of the hot super-Neptune TOI-672 b with NIRPS and HARPS
The Neptunian desert is a distinct lack of Neptune-sized planets at short orbital periods, purportedly carved by photoevaporation and tidal circularisation following high-eccentricity migration.
Osborn Ares +67 more
doaj +1 more source
A Hot Ultraviolet Flare on the M Dwarf Star GJ 674
Abstract As part of the Mega-Measurements of the Ultraviolet Spectral Characteristics of Low-Mass Exoplanetary Systems Hubble Space Telescope (HST) Treasury program, we obtained time-series ultraviolet spectroscopy of the M2.5V star, GJ 674.
Cynthia S. Froning +12 more
openaire +5 more sources
Nearby M Dwarf Stars and the Wide Main Sequence [PDF]
This dissertation addresses the underlying causes for the observed widening of the main sequence for low mass stars and presents the results of three different studies using two different astrophysical observing methods to assess the properties of a ...
Clements, Tiffany D
core +1 more source

