Results 21 to 30 of about 41,311 (309)
Gamma-Ray Bursts from Stellar Collisions [PDF]
The Astrophysical Journal, 1998 Latex, 15 pages, and 2 postscript figures.
Hansen, Brad M. S., Murali, Chigurupati
openaire +2 more sources
Survival of polycyclic aromatic hydrocarbon knockout fragments in the interstellar medium
Nature Communications, 2021 Ion storage rings allow reactions to be studied over orders of magnitude in time, bridging the gap between typical experimental and astronomical timescales.
Michael Gatchell +8 more
doaj +1 more source
EARLY HYDRODYNAMIC EVOLUTION OF A STELLAR COLLISION [PDF]
The Astrophysical Journal, 2014 7 pages, 5 figures (without appendices).
Kushnir, Doron, Katz, Boaz
openaire +2 more sources
Improved treatment of dark matter capture in compact stars
SciPost Physics Proceedings, 2023 Compact stellar objects are promising cosmic laboratories to test the nature of dark matter (DM). DM captured by the strong gravitational field of these stellar remnants transfers kinetic energy to the star during the collision.
Sandra Robles
doaj +1 more source
A comprehensive set of simulations of high-velocity collisions between main sequence stars [PDF]
, 2004 We report on a very large set of simulations of collisions between two main sequence (MS) stars. These computations were done with the ``Smoothed Particle Hydrodynamics'' method. Realistic stellar structure models for evolved MS stars were used. In order
Alexander +123 more
core +3 more sources
Star Formation in Collision Debris: Insights from the modeling of their Spectral Energy Distribution [PDF]
, 2010 During galaxy-galaxy interactions, massive gas clouds can be injected into the intergalactic medium which in turn become gravitationally bound, collapse and form stars, star clusters or even dwarf galaxies.
Appleton, P. N. +6 more
core +5 more sources
, 1998 WFPC-2 images are used to study the central structure of M31, M32, and M33. The dimmer peak, P2, of the M31 double nucleus is centered on the bulge to 0.1", implying that it is the dynamical center of M31.
Bacon R. +11 more
core +2 more sources
Evolution of Stellar Collision Products in Globular Clusters. I. Head‐on Collisions [PDF]
The Astrophysical Journal, 1997 We explore the evolution of collisionally merged stars in the blue straggler region of the HR diagram. The starting models for our stellar evolution calculations are the results of the smoothed particle hydrodynamics (SPH) simulations of parabolic collisions between main sequence stars performed by Lombardi, Rasio and Shapiro (1996).
Sills, Alison +5 more
openaire +2 more sources
Evolution of Stellar Collision Products in Globular Clusters. II. Off‐Axis Collisions [PDF]
The Astrophysical Journal, 2001 25 pages incl. 9 figures (one in colour).
Sills, Alison +4 more
openaire +2 more sources
Distant Echoes of the Milky Way’s Last Major Merger
The Astrophysical Journal, 2023 The majority of the Milky Way’s stellar halo consists of debris from our galaxy’s last major merger, the Gaia-Sausage-Enceladus (GSE). In the past few years, stars from the GSE have been kinematically and chemically studied in the inner 30 kpc of our ...
Vedant Chandra +11 more
doaj +1 more source