Results 81 to 90 of about 64,867 (203)
Revisiting the evolutionary status of massive stars in the central parsec of the Milky Way
Context. Massive stars and their winds strongly affect their environment. For example, they determine the accretion rate on to the Galactic centre (GC) supermassive black hole Sagittarius A* (Sgr A*).
Gormaz-Matamala A. C. +4 more
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A chromosphere is a universal attribute of stars of spectral type later than ~F5. Evolved (K and M) giants and supergiants (including the zeta Aurigae binaries) show extended and highly turbulent chromospheres, which develop into slow massive winds.
A. Brown +139 more
core +1 more source
Investigating Protostellar Accretion (IPA) is a JWST Cycle 1 GO program that uses NIRSpec integral field units and MIRI Medium Resolution Spectrograph to obtain 2.9–28 μ m spectral cubes of young, deeply embedded protostars with luminosities of 0.2–10 ...
Mayank Narang +38 more
doaj +1 more source
Stellar winds from massive stars may be significant sources of cosmic rays (CRs). To investigate this connection, we report a detailed study of gamma-ray emission near the young Milky Way star cluster (≈0.5 Myr old) in the star-forming region RCW 38 and ...
Paarmita Pandey +5 more
doaj +1 more source
We present an analysis of the effects of spectral resolution and aperture scale on derived galaxy properties using far-ultraviolet (FUV) spectra of local star-forming galaxies from the International Ultraviolet Explorer ( R ∼ 250, field of view (FOV ...
Ilyse Clark +4 more
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Relativistic Stellar-Wind Torques
Solar wind-induced torque calculated considering special and general relativistic effects, extending method to pulsar rotational ...
openaire +1 more source
Low energy gamma ray emission from the Cygnus OB2 association [PDF]
According to our newly developed model of gamma-ray emission from chaotic early-type stellar winds, we predict the combined gamma-ray flux from the circumstellar winds of many very luminous early-type stars in the Cyg OB2 association can be detectable by
Chen, Wan, White, Richard L.
core +1 more source
Abstract : WITH CLASS G main sequence and M-giant stars are given for various interst llar environments. The supersonic wind from a class G star undergoes a shock transition to subsonic flow at a radial distance of 100 - 1,000 a.u. and may extend many times farther as a subsonic flow. Thic storms. Open-ended Terms: Stellar Wind.
openaire +1 more source
First Statistical Detection of Mg ii-traced Cool Gas Outflows with JWST toward Cosmic Dawn
Galactic-scale outflows are a crucial component of galaxy evolution, yet their properties in the early Universe remain poorly constrained. We present the first statistical investigation of Mg ii -traced cool gas outflows in galaxies spanning a wide ...
Cheqiu Lyu +11 more
doaj +1 more source
Rotational Evolution of Classical T Tauri Stars: Models and Observations
We developed a grid of stellar rotation models for low-mass and solar-type classical T Tauri stars (CTTS; 0.3 M _⊙ < M _* < 1.2 M _⊙ ). These models incorporate the star–disk interaction and magnetospheric ejections to investigate the evolution of the ...
Javier Serna +19 more
doaj +1 more source

