Results 41 to 50 of about 1,100,727 (344)
Clump formation through colliding stellar winds in the Galactic Centre [PDF]
Proceedings of the International Astronomical Union, 2015 We study the process of clump formation from hydrodynamic instabilities in stellar wind collisions, using analytical and numerical techniques. We show that the cloud G2 in the Galactic Centre could have been formed in this way, with the most promising ...
Diego Calderón +6 more
semanticscholar +1 more source
The Nature of Stellar Winds in the Star-Disk Interaction [PDF]
, 2007 Stellar winds may be important for angular momentum transport from accreting T Tauri stars, but the nature of these winds is still not well-constrained.
Bisnovatyi-Kogan +4 more
core +1 more source
The interaction of multiple stellar winds in stellar clusters: potential flow
, 2018 While several studies have investigated large-scale cluster winds resulting from an intra-cluster interaction of multiple stellar winds, as yet they have not provided details of the bordering flows inside a given cluster.
Fichtner, Horst +4 more
core +1 more source
The Astrophysical Journal, 2023 Many of the short-lived radioactive nuclei that were present in the early solar system can be produced in massive stars. In the first paper in this series, we focused on the production of ^26 Al in massive binaries.
Hannah E. Brinkman +4 more
doaj +1 more source
Stellar Mass Loss-Driven Wind Models of Elliptical Galaxies?
, 1994 Recent claims in the literature (Bressan, Chiosi & Fagotto 1994) that the epoch describing the onset of galactic winds in spheroidal star systems has been severely overestimated in the past, due to the neglect of energy deposited in the interstellar ...
Gibson, Brad K.
core +1 more source
Stellar feedback efficiencies: supernovae versus stellar winds [PDF]
, 2015 The final, definitive version of this paper has been published in Monthly Notices of the Royal Astronomical Society, Vol. 456(1): 710-730, February 2016, DOI: 10.1093/mnras/stv2699, published by Oxford University Press on behalf of MNRAS.
K. Fierlinger +7 more
semanticscholar +1 more source
A FUSE View of the Stellar Winds of Planetary Nebula Central Stars
, 2009 Since the IUE satellite produced a vast collection of high-resolution UV spectra of central stars of planetary nebulae (CSPNe), there has not been any further systematic study of the stellar winds of these stars. The high spectral resolution, sensitivity
Derck Massa +3 more
core +1 more source
Accretion in supergiant High Mass X-ray Binaries
EPJ Web of Conferences, 2014 Supergiant High Mass X-ray Binary systems (sgHMXBs) consist of a massive, late type, star and a neutron star. The massive stars exhibits strong, radiatively driven, stellar winds.
Manousakis Antonios +2 more
doaj +1 more source
The Astrophysical Journal, 2022 We perform three-dimensional (3D) magnetohydrodynamic simulations of magnetospheric accretion in a T Tauri star to study the accretion and wind structures in the close vicinity of the star.
Shinsuke Takasao +3 more
doaj +1 more source
Star/disk interaction and angular momentum evolution model for solar-like stars
EPJ Web of Conferences, 2014 The magnetic field in young stellar object is undoubtedly the most important component when one dealing with the angular momentum evolution. It controls this latter one from the pre-main sequence, during the so-called disk locking phase where the stars ...
Gallet Florian
doaj +1 more source