Results 11 to 20 of about 338 (243)

WIYN Open Cluster Study. LXXXVII. Hubble Space Telescope Ultraviolet Detection of Hot White Dwarf Companions to Blue Lurkers in M67

open access: yesThe Astrophysical Journal, 2023
We present the results of our Hubble Space Telescope far-ultraviolet survey of the blue lurkers (BLs) in M67. We find evidence for two white dwarf (WD) companions among the BLs that are indicative of mass transfer from an evolved companion, one in WOCS ...
Andrew C. Nine   +3 more
doaj   +1 more source

Blue straggler production in globular clusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2004
7 pages, 6 figures; MNRAS in ...
DAVIES M.   +2 more
openaire   +2 more sources

BLUE STRAGGLERS AFTER THE MAIN SEQUENCE [PDF]

open access: yesThe Astrophysical Journal, 2009
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. We found that the blue straggler progeny populate the colour-magnitude diagram slightly blueward of the red giant branch and between 0.2 and 1 ...
Sills, A.   +2 more
openaire   +3 more sources

BD+43° 3654 – a blue straggler? [PDF]

open access: yesAstronomy & Astrophysics, 2008
4 pages, 1 figure, accepted for publication in A&A ...
Gvaramadze, V. V., Bomans, D. J.
openaire   +2 more sources

Primordial binary evolution and blue stragglers [PDF]

open access: yesProceedings of the International Astronomical Union, 2009
AbstractBlue stragglers have been found in all populations. They are important in both stellar evolution and stellar population synthesis. Much evidence shows that blue stragglers are relevant to primordial binaries. Here, we summarize the links between binary evolution and blue stragglers, describe the characteristics of blue stragglers originating ...
Chen, X., Han, Z.
openaire   +4 more sources

Building Blue Stragglers with Stellar Collisions [PDF]

open access: yesProceedings of the International Astronomical Union, 2007
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 ...
Glebbeek, E., Pols, O.R.
openaire   +3 more sources

SPINNING LIKE A BLUE STRAGGLER: THE POPULATION OF FAST ROTATING BLUE STRAGGLER STARS IN ω CENTAURI [PDF]

open access: yesThe Astrophysical Journal, 2014
By using high-resolution spectra acquired with FLAMES-GIRAFFE at the ESO/VLT, we measured radial and rotational velocities for 110 Blue Straggler stars (BSSs) in Omega Centauri, the globular cluster-like stellar system harboring the largest known BSS population. According to their radial velocities, 109 BSSs are members of the system.
MUCCIARELLI, ALESSIO   +5 more
openaire   +2 more sources

SPECTRAL INVESTIGATION OF FIELD BLUE STRAGGLERS

open access: yesOdessa Astronomical Publications, 2017
Field blue stragglers are counterparts of cluster blue stragglers. They were selected by Olsen in base of specific Stromgren indices among bright metal-deficient early F dwarfs. For some stars from this list, the high-resolution and high S/N CCD spectra
I. V. Chernyshova
doaj   +1 more source

Chemical abundances and evolutionary status of some lambda Bootis type stars and FBSwl

open access: yesOdessa Astronomical Publications, 2017
Comparative analysis of chemical abundances in the atmospheres of lambda Bootis type stars and FBSwl (field blue stragglers week lined) is presented. Evolutionary status of these metal deficient stars is discussed.
I. V. Chernyshova
doaj   +1 more source

The lithium abundance of M67 blue stragglers - A constraint on the blue straggler phenomenon

open access: yesThe Astrophysical Journal, 1991
Upper limits have been placed on the line strength of the 6707 A Li I resonance doublet in seven blue stragglers in M67. The corresponding upper limits on abundances range from log N(Li) less than about 1.3 to less than about 2.3. This result is significantly below the level of log N(Li) about 3.1 + or {minus} 0.1 found in field main-sequence stars of ...
C. J. Pritchet, J. W. Glaspey
openaire   +1 more source

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