Results 21 to 30 of about 26,349 (244)

Constraints on the Distance Moduli, Helium, and Metal Abundances, and Ages of Globular Clusters from Their RR Lyrae and Non-variable Horizontal Branch Stars. II. Multiple Stellar Populations in 47 Tuc, M3, and M13 [PDF]

open access: yes, 2017
We present a new set of horizontal branch (HB) models computed with the MESA stellar evolution code. The models adopt α-enhanced Asplund et al. metal mixtures and include the gravitational settling of He. They are used in our HB population synthesis tool
P. Denissenkov   +3 more
semanticscholar   +1 more source

VVV Survey of Blue Horizontal Branch Stars in the Bulge–Halo Transition Region of the Milky Way [PDF]

open access: yesAstrophysical Journal, 2018
We characterize the population of blue horizontal branch (BHB) stars in the bulge–halo transition region of the Milky Way using the VISTA Variables in the Vía Láctea (VVV) ESO Public Survey data.
K. Montenegro   +6 more
semanticscholar   +1 more source

Mapping the anisotropic Galactic stellar halo with blue horizontal branch stars [PDF]

open access: yesAstronomy & Astrophysics
We used Legacy Survey photometric data to probe the stellar halo in multiple directions of the sky using a probabilistic methodology to identify blue horizontal branch (BHB) stars. The measured average radial density profile follows a double power law in
Joao A. S. Amarante   +2 more
semanticscholar   +1 more source

SHOTGLAS: I. The ultimate spectroscopic census of extreme horizontal branch stars in ω Centauri [PDF]

open access: yes, 2018
The presence of extreme horizontal branch (EHB) and blue hook stars in some Galactic globular clusters (GGCs) constitutes one of the remaining mysteries of stellar evolution.
M. Latour   +4 more
semanticscholar   +1 more source

Multiple Stellar Populations along the Red Horizontal Branch and Red Clump of Globular Clusters [PDF]

open access: yes, 2020
We exploit multiband Hubble Space Telescope photometry to investigate multiple populations (MPs) along the red horizontal branches (HBs) and red clumps of 14 metal-rich globular clusters (GCs), including 12 Milky Way GCs and the Magellanic Cloud GCs NGC ...
E. Dondoglio   +7 more
semanticscholar   +1 more source

CONSTRAINTS ON THE DISTANCE MODULI, HELIUM AND METAL ABUNDANCES, AND AGES OF GLOBULAR CLUSTERS FROM THEIR RR LYRAE AND NON-VARIABLE HORIZONTAL-BRANCH STARS. I. M3, M15, AND M92 [PDF]

open access: yes, 2016
Up-to-date isochrones, zero-age horizontal-branch (ZAHB) loci, and evolutionary tracks for core He-burning stars are applied to the color–magnitude diagrams of M3, M15, and M92, focusing in particular on their RR Lyrae populations.
D. VandenBerg   +2 more
semanticscholar   +1 more source

Multiple Stellar Populations in Asymptotic Giant Branch Stars of Galactic Globular Clusters [PDF]

open access: yes, 2021
Multiple stellar populations (MPs) are a distinct characteristic of globular clusters (GCs). Their general properties have been widely studied among main-sequence, red giant branch (RGB), and horizontal branch (HB) stars, but a common framework is still ...
E. Lagioia   +10 more
semanticscholar   +1 more source

Characterizing stellar halo populations II: the age gradient in blue horizontal-branch stars [PDF]

open access: yes, 2016
The distribution of Milky Way halo blue horizontal-branch (BHB) stars is examined using action-based extended distribution functions (EDFs) that describe the locations of stars in phase space, metallicity, and age.
P. Das, Angus Williams, J. Binney
semanticscholar   +1 more source

RR Lyrae stars and the horizontal branch of NGC 5904 (M5) [PDF]

open access: yes, 2016
We report the distance and [Fe/H] value for the globular cluster NGC 5904 (M5) derived from the Fourier decomposition of the light curves of selected RRab and RRc stars.
A. Arellano Ferro   +5 more
semanticscholar   +1 more source

Level of helium enhancement among M3's horizontal-branch stars [PDF]

open access: yes, 2016
(Abridged) The color and luminosity distribution of horizontal branch (HB) stars in globular clusters are sensitive probes of their original helium abundances.
A. Valcarce   +4 more
semanticscholar   +1 more source

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