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A New Spin on the Problem of Horizontal‐Branch Gaps: Stellar Rotation along the Blue Horizontal Branch of Globular Cluster M13

Behr, Bradford B. and Djorgovski, S. G. and Cohen, Judith G. and McCarthy, James K. and Côté, Patrick and Piotto, Giampaolo and Zoccali, Manuela (2000) A New Spin on the Problem of Horizontal‐Branch Gaps: Stellar Rotation along the Blue Horizontal Branch of Globular Cluster M13. Astrophysical Journal, 528 (2). pp. 849-853. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20190524-141458208

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Abstract

We have determined the projected rotational velocities of 13 blue horizontal-branch (BHB) stars in the globular cluster M13 via rotational broadening of metal absorption lines. Our sample spans the photometric gap observed in the horizontal-branch distribution at T_(eff) 11,000 K and reveals a pronounced difference in stellar rotation on either side of this feature—blueward of the gap, all the stars show modest rotations, v sin i < 10 km s^(-1), while to the red side of the gap, we confirm the more rapidly rotating population (v sin i ≃ 40 km s^(-1)) previously observed by R. C. Peterson and coworkers. Taken together with these prior results, our measurements indicate that a star's rotation is indeed related to its location along the HB, although the mechanism behind this correlation remains unknown. We explore possible connections between stellar rotation and mass-loss mechanisms which influence the photometric morphology of globular cluster HBs.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/308219DOIArticle
https://arxiv.org/abs/astro-ph/9907211arXivDiscussion Paper
ORCID:
AuthorORCID
Djorgovski, S. G.0000-0002-0603-3087
Cohen, Judith G.0000-0002-8039-4673
Côté, Patrick0000-0003-1184-8114
Alternate Title:A New Spin on the Problem of HB Gaps: Stellar Rotation along the Blue Horizontal Branch of Globular Cluster M13
Additional Information:© 2000 The American Astronomical Society. Received 1999 May 3; accepted 1999 August 24. Based on observations obtained at the W. M. Keck Observatory, which is operated jointly by the California Institute of Technology and the University of California. Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555. 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. S. G. D. was supported, in part, by the Bressler Foundation, and STScI grant GO-7470. J. G. C. acknowledges support by NSF grant AST-9819614. P. C. gratefully acknowledges support provided by the Sherman M. Fairchild Foundation. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France.
Funders:
Funding AgencyGrant Number
NASANAS 5-26555
Bressler FoundationUNSPECIFIED
NASAGO-7470
NSFAST-9819614
Sherman Fairchild FoundationUNSPECIFIED
Subject Keywords:globular clusters : general - globular clusters : individual (NGC 6205) - stars : horizontal-branch - stars : rotation
Issue or Number:2
Record Number:CaltechAUTHORS:20190524-141458208
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190524-141458208
Official Citation:Bradford B. Behr et al 2000 ApJ 528 849
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95795
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:24 May 2019 21:22
Last Modified:06 Nov 2019 23:51

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