Results 141 to 150 of about 412,693 (262)
Fundamental Parameters for Central Stars of 103 Infrared Bow Shock Nebulae
Stellar bow shock nebulae are arcuate shock fronts formed by the interaction of radiation-driven stellar winds and the relative motion of the ambient interstellar material.
Nikhil Patten +18 more
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ASPITZER SPACE TELESCOPEATLAS OF ω CENTAURI: THE STELLAR POPULATION, MASS LOSS, AND THE INTRACLUSTER MEDIUM [PDF]
Martha L. Boyer +6 more
openalex +1 more source
A Semi-analytical Model for Stellar Evolution in AGN Disks
Disks of gas accreting onto supermassive black holes may host numerous stellar-mass objects, formed within the disk or captured from a nuclear star cluster.
Alexander J. Dittmann, Matteo Cantiello
doaj +1 more source
Effects of Dark Matter Self-interactions on Sagittarius and its Stream
This work explores how assumptions regarding the particle-physics nature of dark matter can alter the evolution of the Sagittarius (Sgr) dwarf spheroidal galaxy and its expansive stellar stream.
Connor Hainje +3 more
doaj +1 more source
Atmospheric Mass Loss from Hot Jupiters Irradiated by Stellar Superflares [PDF]
Д. В. Бисикало +4 more
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We study the effect of stellar evolution on the dispersal of protoplanetary disks by performing one-dimensional simulations of long-term disk evolution.
Ayano Komaki, Naoki Yoshida
doaj +1 more source
The dependence of mass loss on the basic stellar parameters [PDF]
H. J. G. L. M. Lamers
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Evolution of the Convective Core Mass during the Main Sequence
We construct a semianalytical model that describes the convective core mass evolution of massive stars experiencing mass loss during the main-sequence stage.
Minori Shikauchi +2 more
doaj +1 more source
Intense accretion and mass loss of a very low mass young stellar object [PDF]
M. Fernández, F. Comerón
openalex +1 more source

