Results 31 to 40 of about 4,300 (180)

Overfitting Affects the Reliability of Radial Velocity Mass Estimates of the V1298 Tau Planets

open access: yesThe Astronomical Journal, 2023
Mass, radius, and age measurements of young (≲100 Myr) planets have the power to shape our understanding of planet formation. However, young stars tend to be extremely variable in both photometry and radial velocity (RV) measurements, which makes ...
Sarah Blunt   +25 more
doaj   +1 more source

Multiple views of magnetism in cool stars [PDF]

open access: yes, 2012
Magnetic fields are regarded as a crucial element for our understanding of stellar physics. They can be studied with a variety of methods which provide complementary - and sometimes contradictory - information about the structure, strength and dynamics ...
Arzoumanian   +24 more
core   +3 more sources

Asteroseismic Signature of a Large Active Region

open access: yesFrontiers in Astronomy and Space Sciences, 2019
Axisymmetric magnetic activity on the Sun and sun-like stars increases the frequencies of the modes of acoustic oscillation. However, it is unclear how a corotating patch of activity affects the oscillations, since such a perturbation is unsteady in the ...
Emanuele Papini   +2 more
doaj   +1 more source

Temperature-Pressure Profile of the hot Jupiter HD 189733b from HST Sodium Observations: Detection of Upper Atmospheric Heating [PDF]

open access: yes, 2012
We present transmission spectra of the hot Jupiter HD 189733b taken with the Space Telescope Imaging Spectrograph aboard HST. The spectra cover the wavelength range 5808-6380 Ang with a resolving power of R=5000. We detect absorption from the NaI doublet
Ballester, Gilda E.   +6 more
core   +1 more source

High Tide or Riptide on the Cosmic Shoreline? A Water-rich Atmosphere or Stellar Contamination for the Warm Super-Earth GJ 486b from JWST Observations

open access: yesThe Astrophysical Journal Letters, 2023
Planets orbiting M-dwarf stars are prime targets in the search for rocky exoplanet atmospheres. The small size of M dwarfs renders their planets exceptional targets for transmission spectroscopy, facilitating atmospheric characterization.
Sarah E. Moran   +23 more
doaj   +1 more source

Formation of starspots in self-consistent global dynamo models: Polar spots on cool stars [PDF]

open access: yes, 2014
Observations of cool stars reveal dark spot-like features on their surfaces. Compared to sunspots, starspots can be bigger or cover a larger fraction of the stellar surface.
Christensen, Ulrich R.   +3 more
core   +1 more source

Starspot photometry with robotic telescopes [PDF]

open access: yesAstronomy and Astrophysics Supplement Series, 1997
We report on the progress of our ongoing photometric monitoring program of spotted late-type stars with automatic photoelectric telescopes (APTs) on Mt. Hopkins in Arizona and on Mt. Etna in Sicily. We present 9 250 differential UBV and/or observations for altogether 23 chromospherically active stars, singles and binaries, pre main sequence and post ...
K. G. Strassmeier   +3 more
openaire   +1 more source

Measuring the Temperature of Starspots from Multi-filter Photometry

open access: yesThe Astronomical Journal, 2023
Using simultaneous multi-filter observations during the transit of an exoplanet around a K dwarf star, we determine the temperature of a starspot through modeling the radius and position with wavelength-dependent spot contrasts.
Maria C. Schutte   +7 more
doaj   +1 more source

Photospheric activity, rotation and magnetic interaction in LHS 6343 A [PDF]

open access: yes, 2013
Context. The Kepler mission has recently discovered a brown dwarf companion transiting one member of the M4V+M5V visual binary system LHS 6343 AB with an orbital period of 12.71 days. Aims.
Herrero, E.   +4 more
core   +1 more source

Benchmarking pre-main sequence stellar evolutionary tracks using disk-based dynamical stellar masses

open access: yesAstronomy & Astrophysics
Stellar masses are a fundamental property to understand models of pre-main sequence evolution, but their values derived from Hertzsprung–Russell (HR) diagrams are strongly model dependent.
Zallio Luigi   +16 more
doaj   +1 more source

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