Results 1 to 10 of about 5,234 (215)
Fast rotating blue stragglers prefer loose clusters [PDF]
Blue stragglers are anomalously luminous core hydrogen-burning stars formed through mass-transfer in binary/triple systems and stellar collisions. Their physical and evolutionary properties are largely unknown and unconstrained.
Francesco R. Ferraro +11 more
doaj +5 more sources
A binary-related origin mediated by environmental conditions for blue straggler stars [PDF]
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 +4 more sources
Explaining the Praesepe blue straggler HD 73666 [PDF]
The blue straggler phenomenon is not yet well explained by current theory; however, evolutionary models of star clusters call for a good knowledge of it.
Adams +59 more
core +6 more sources
Blue Stragglers After the Main Sequence [PDF]
We study the post-main sequence evolution of products of collisions between main sequence stars (blue stragglers), with particular interest paid to the horizontal branch and asymptotic giant branch phases.
Alison Sills +22 more
core +4 more sources
Ecology of Blue Straggler Stars [PDF]
Ecology of Blue Straggler Stars, H.M.J. Boffin, G. Carraro & G.
H. M. J. Boffin, G. Carraro, G. Beccari
+6 more sources
WOCS 4540: Detailed Analysis of a very Long Orbital Period Blue Straggler [PDF]
WOCS 4540 is the longest orbital period ( P _orb = 3030 days) blue straggler star (BSS)—white dwarf (WD) pair in the old open cluster NGC 188. It also contains one of the most luminous BSS in the cluster.
Meng Sun, Robert D. Mathieu
doaj +2 more sources
Blue Straggler Formation in Clusters [PDF]
Blue stragglers are thought to be formed from the merger or coalescence of two stars, but the details of their formation in clusters has been difficult to disentangle.
Sills, Alison
core +2 more sources
Fast-rotating blue straggler stars in the globular cluster NGC 1851 [PDF]
We studied the rotational velocities of a sample of blue straggler stars (BSSs) and reference stars belonging to the Galactic globular cluster NGC 1851 using high-resolution spectra acquired with FLAMES-GIRAFFE at the ESO/VLT. After field decontamination
Billi A. +6 more
doaj +2 more sources
Unveiling Bifurcated Blue Straggler Sequences in NGC 2173: Insights from Binary Evolution [PDF]
Identifying bifurcated blue straggler (BS) sequences in color–magnitude diagrams (CMDs) of star clusters has long been regarded as a powerful diagnostic for distinguishing different BS formation mechanisms.
Li Wang +5 more
doaj +2 more sources
Building Blue Stragglers with Stellar Collisions [PDF]
AbstractThe 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 product was completely mixed during the collision.It is known from hydrodynamical simulations of ...
E. Glebbeek, Onno R. Pols
openalex +4 more sources

