Results 41 to 50 of about 5,593,868 (306)

THE FATE OF STELLAR MASS LOSS IN CENTRAL CLUSTER GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2011
ApJ Letters, in press, 4 pages, 1 ...
Voit, G. Mark, Donahue, Megan
openaire   +2 more sources

Continuous stellar mass-loss in

open access: yes, 2001
We present an N-body computer code -aimed at studies of galactic dynamics - with a CPU-efficient algorithm for a continuous (i.e. time-dependent) stellar mass-loss. First, we summarize available data on stellar mass-loss and derive the long-term (20 Gyr)
F. Combes, B. Jungwiert, J. Palouš
core   +1 more source

Extreme Tidal Stripping May Explain the Overmassive Black Hole in Leo I: A Proof of Concept

open access: yesThe Astrophysical Journal Letters, 2023
A recent study found dynamical evidence of a supermassive black hole of ∼3 × 10 ^6 M _⊙ at the center of Leo I, the most distant dwarf spheroidal galaxy of the Milky Way. This black hole, comparable in mass to the Milky Way’s Sgr A*, places the system >2
Fabio Pacucci, Yueying Ni, Abraham Loeb
doaj   +1 more source

The initial/final mass relation for stellar evolution with mass loss [PDF]

open access: yesInternational Astronomical Union Colloquium, 1981
The relation between initial and final masses is discussed under consideration of changing theoretical concepts and new empirical data on masses of white dwarfs and nuclei of planetary nebulae. It is concluded that presently adopted schemes of evolution need revision, and that no universal relation exists.The strongest evidence for large amounts of ...
openaire   +1 more source

Magnetism in High-Mass Stars

open access: yesGalaxies, 2023
Magnetism is a ubiquitous property of astrophysical plasmas, yet stellar magnetism still remains far from being completely understood. In this review, we describe recent observational and modelling efforts and progress to expand our knowledge of the ...
Zsolt Keszthelyi
doaj   +1 more source

Detection of mass loss in stellar chromospheres

open access: yesThe Astrophysical Journal, 1980
IUE observations of 47 cool giants have been made in a search for the onset of expansion in the Mg II h and k emission cores. It is found that, in a statistical sense, the longward emission peak becomes dominant above a velocity dividing line in the H-R diagram, which lies close to a temperature dividing line reported by Linsky and Haisch (1979).
R. E. Stencel, D. J. Mullan
openaire   +1 more source

Influence of surface stressing on stellar coronae and winds [PDF]

open access: yes, 2013
STFC funding has supported this research.The large-scale field of the Sun is well represented by its lowest energy (or potential) state. Recent observations, by comparison, reveal that many solar-type stars show large-scale surface magnetic fields that ...
Morin, J.   +12 more
core   +1 more source

Solid Pseudopapillary Neoplasm of the Pancreas in Children and Adolescents: Expert Recommendations

open access: yesPediatric Blood &Cancer, EarlyView.
ABSTRACT Solid pseudopapillary neoplasm of the pancreas (SPN) is a rare low‐grade malignant exocrine pancreatic tumor, mostly discovered during the second decade of life in females, with a very good prognosis, provided microscopically complete surgical excision is achieved.
Sabine Irtan   +18 more
wiley   +1 more source

Quasi-Keplerian Be-star Disks with Mimicking Viscosity

open access: yesThe Astrophysical Journal
Classical Be stars are fast-rotating B-type stars with gaseous quasi-Keplerian disks formed by equatorial ejection of material. While the viscous decretion disk (VDD) model reproduces many observed properties, the role of radiative line driving in ...
Michel Curé   +7 more
doaj   +1 more source

CAST constraints on the axion-electron coupling [PDF]

open access: yes, 2013
In non-hadronic axion models, which have a tree-level axion-electron interaction, the Sun produces a strong axion flux by bremsstrahlung, Compton scattering, and axiorecombination, the "BCA processes." Based on a new calculation of this flux, including ...
Barth, Klaus   +121 more
core   +1 more source

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