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Stellar Collisions in Galactic Nuclei: Impact on Destructive Events Near a Supermassive Black Hole [PDF]

open access: greenThe Astrophysical Journal, 2023
The centers of galaxies host both a supermassive black hole and a dense stellar cluster. Such an environment should lead to stellar collisions, possibly at very high velocities so that the total energy involved is of the same order as supernova ...
Shmuel Balberg, Gilad Yassur
doaj   +2 more sources

Stellar collisions in globular clusters: the origin of multiple stellar populations [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2022
ABSTRACT Two generations of stars, G1 and G2, typically populate Galactic globular clusters (GCs). The origin of G2 stars is unclear. We uncover two empirical dependencies between GC characteristics, which can be explained by the formation of G2 main-sequence (MS) stars due to collision/merging of their primordial counterparts (G1).
В. В. Кравцов   +3 more
openalex   +3 more sources

Building Blue Stragglers with Stellar Collisions [PDF]

open access: yesProceedings of the International Astronomical Union, 2007
The evolution of stellar collision products in cluster simulations has usually been modelled using simplified prescriptions. Such prescriptions either replace the collision product with an (evolved) main sequence star, or assume that the collision ...
Glebbeek, E., Pols, O. R.
core   +3 more sources

Magnetic Field Amplification during Stellar Collisions between Low-mass Stars

open access: goldThe Astrophysical Journal Letters
Blue straggler stars in stellar clusters appear younger and bluer than other cluster members, offering a unique opportunity to understand the stellar dynamics and populations within their hosts.
Taeho Ryu   +4 more
doaj   +2 more sources

Stellar Collisions and Pulsar Planets [PDF]

open access: green, 2000
Tex, 17 pages, including 6 postscript figures To appear in: Stellar Collisions, Mergers and their Consequences, ASP Conference Series, Ed.
Brad M. S. Hansen
openalex   +3 more sources

Simulations of Stellar Collisions Involving Pre-Main Sequence Stars [PDF]

open access: yesThe Astrophysical Journal, 2005
In this paper, we present the results of smoothed particle hydrodynamic (SPH) simulations of collisions between pre-main sequence stars and a variety of other kinds of stars. Simulations over a range of impact parameters and velocities were performed. We
Alison Sills   +3 more
core   +3 more sources

A binary-related origin mediated by environmental conditions for blue straggler stars [PDF]

open access: yesNature Communications
Blue stragglers are anomalously massive core hydrogen-burning stars that, according to the theory of single star evolution, should not exist. They are suspected to form in mass-enhancement processes, involving binary evolution or stellar collisions.
Francesco R. Ferraro   +9 more
doaj   +2 more sources

Multiple Populations in Globular Clusters: The Possible Contributions of Stellar Collisions [PDF]

open access: bronze, 2010
Globular clusters were thought to be simple stellar populations, but recent photometric and spectroscopic evidence suggests that the clusters' early formation history was more complicated.
Alison Sills   +53 more
core   +3 more sources

On the Orbital Effects of Stellar Collisions in Galactic Nuclei: Tidal Disruption Events and Ejected Stars [PDF]

open access: greenThe Astrophysical Journal Letters
Dense stellar clusters surround the supermassive black holes (SMBH) in galactic nuclei. Interactions within the cluster can alter the stellar orbits, occasionally driving a star into the SMBH’s tidal radius, where it becomes ruptured, or expelling a star
Sanaea C. Rose, Brenna Mockler
doaj   +2 more sources

A Supernova Remnant Collision with a Stellar Wind [PDF]

open access: greenThe Astrophysical Journal, 2003
Numerical simulations of the interaction between supernova ejecta and a stellar wind are presented. We follow the temporal evolution of the shock fronts that are formed through such an interaction and determine the velocities, temperatures and densities.
P. F. Velázquez   +2 more
openalex   +4 more sources

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