CaltechAUTHORS
  A Caltech Library Service

Rotations and Abundances of Blue Horizontal-Branch Stars in Globular Cluster M15

Behr, Bradford B. and Cohen, Judith G. and McCarthy, James K. (2000) Rotations and Abundances of Blue Horizontal-Branch Stars in Globular Cluster M15. Astrophysical Journal, 531 (1). L37-L40. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20190524-135043421

[img] PDF - Published Version
See Usage Policy.

55Kb
[img] PDF - Accepted Version
See Usage Policy.

105Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20190524-135043421

Abstract

High-resolution optical spectra of 18 blue horizontal-branch stars in the globular cluster M15 indicate that their stellar rotation rates and photospheric compositions vary strongly as a function of effective temperature. Among the cooler stars in the sample, at T_(eff) ~ 8500 K, metal abundances are in rough agreement with the canonical cluster metallicity, and the v sin i rotations appear to have a bimodal distribution, with eight stars at v sin i < 15 km s^(-1) and two stars at v sin i ~ 35 km s^(-1). Most of the stars at T_(eff) ≥ 10,000 K, however, are slowly rotating, v sin i < 7 km s^(-1), and their iron and titanium are enhanced by a factor of 300 to solar abundance levels. Magnesium maintains a nearly constant abundance over the entire range of T_(eff), and helium is depleted by factors of 10-30 in three of the hotter stars. Diffusion effects in the stellar atmospheres are the most likely explanation for these large differences in composition. Our results are qualitatively very similar to those previously reported for M13 and NGC 6752, but with even larger enhancement amplitudes, presumably due to the increased efficiency of radiative levitation at lower intrinsic [Fe/H]. We also see evidence for faster stellar rotation explicitly preventing the onset of the diffusion mechanisms among a subset of the hotter stars.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/312524DOIArticle
https://arxiv.org/abs/astro-ph/0002119arXivDiscussion Paper
ORCID:
AuthorORCID
Cohen, Judith G.0000-0002-8039-4673
Additional Information:© 2000 The American Astronomical Society. Received 1999 November 25; accepted 2000 January 12; published 2000 February 9. Based in large part on observations obtained at the W. M. Keck Observatory, which is operated jointly by the California Institute of Technology and the University of California. These observations would not have been feasible without the HIRES spectrograph and the Keck I telescope. We are indebted to Jerry Nelson, Gerry Smith, Steve Vogt, and many others for making such marvelous machines, to the W. M. Keck Foundation for making it happen, and to a bevy of Keck observing assistants for making them work. J. G. C. and B. B. B. are grateful for support from NSF grant AST 98-19614.
Funders:
Funding AgencyGrant Number
W. M. Keck FoundationUNSPECIFIED
NSFAST 98-19614
Subject Keywords:globular clusters: general—globular clusters: individual (NGC 7078)—stars: abundances—stars: horizontal-branch—stars: rotation
Issue or Number:1
Record Number:CaltechAUTHORS:20190524-135043421
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190524-135043421
Official Citation:Bradford B. Behr et al 2000 ApJ 531 L37
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95792
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:24 May 2019 21:16
Last Modified:03 Oct 2019 21:16

Repository Staff Only: item control page