Results 31 to 40 of about 765,419 (288)

Visual Orbits and Alignments of Planet-hosting Binary Systems

open access: yesThe Astronomical Journal, 2023
Roughly half of Solar-type planet hosts have stellar companions, so understanding how these binary companions affect the formation and evolution of planets is an important component to understanding planetary systems overall.
Kathryn V. Lester   +9 more
doaj   +1 more source

Asteroseismic masses of retired planet-hosting A-stars using SONG

open access: yes, 2020
To better understand how planets form, it is important to study planet occurrence rates as a function of stellar mass. However, estimating masses of field stars is often difficult.
Kjeldsen, H   +11 more
core   +1 more source

Spectroscopic metallicities for planet-host stars: Extending the samples [PDF]

open access: yesAstronomy & Astrophysics, 2005
Accepted for publication in A&A; Replaced by new version on 19/04/2005: corrections in Tables 1 and ...
Santos, N. C.   +6 more
openaire   +2 more sources

Close-by planets and flares in their host stars [PDF]

open access: yesAstronomy & Astrophysics, 2018
Context. The interaction between the magnetic fields of late-type stars and their close-by planets may produce stellar flares as observed in active binary systems. However, in spite of several claims, conclusive evidence is still lacking. Aim. We estimate the magnetic energy available in the interaction using analytical models to provide an upper bound
openaire   +3 more sources

Lucky imaging of transiting planet host stars with LuckyCam [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
We obtained high-resolution, high-contrast optical imaging in the SDSS $i'$ band with the LuckyCam camera mounted on the 2.56m Nordic Optical Telescope, to search for faint stellar companions to 16 stars harbouring transiting exoplanets. The Lucky Imaging technique uses very short exposures to obtain near diffraction-limited images yielding sub ...
Faedi, F.   +9 more
openaire   +3 more sources

CHEMICAL IMPRINTS IN ATMOSPHERIC ABUNDANCES IN PLANET- HOSTING STARS

open access: yesOdessa Astronomical Publications, 2019
We examined 12 planet-hosting stars based on homogeneous spectral data (obtained with the SOPHIE echelle spectrograph with R = 75,000 at the OHP, France) and using uniform techniques for determination of parameters and abundances of a series of elements (
T. Mishenina, N. Basak, V. Kovtyukh
doaj   +1 more source

MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert

open access: yesThe Astronomical Journal, 2023
We analyze the MOA-2020-BLG-208 gravitational microlensing event and present the discovery and characterization of a new planet, MOA-2020-BLG-208Lb, with an estimated sub-Saturn mass.
Greg Olmschenk   +82 more
doaj   +1 more source

Circulating microRNA signatures of cachexia and cancer in Canis familiaris as a comparative oncology model for human disease

open access: yesMolecular Oncology, EarlyView.
Circulating microRNAs as biomarkers of cachexia and sex‐specific cancer in senior dogs. In 25 client‐owned dogs, four circulating miRNAs (miR‐15a, miR‐15b, miR‐16, miR‐140) were downregulated in cachexia, with miR‐16 the strongest individual biomarker (AUC = 0.899).
Soon‐Seok Park   +6 more
wiley   +1 more source

From energy provision to protein synthesis: Tunnelling nanotubes as mediators of intercellular metabolic cooperation in cancer

open access: yesFEBS Open Bio, EarlyView.
The cytoskeleton‐mediated transport of mitochondria via tunnelling nanotubes restores respiration, increases ATP production, rescues cells from apoptosis, activates the AKT/mTOR signalling pathway, promotes cell migration and invasiveness, contributes to cancer progression and treatment resistance.
Stanislava Martínková, Jan Trnka
wiley   +1 more source

Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-dependent Sub-Neptune Formation

open access: yesThe Astronomical Journal
M dwarfs are the most common sites of planet formation in the Milky Way. Planet occurrence and composition are closely linked with the availability of metals in protoplanetary disks, which can be probed by measuring the metallicity of planet host stars ...
Emma V. Turtelboom   +8 more
doaj   +1 more source

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