New rotation periods in the open cluster NGC 1039 (M 34), and a derivation of its gyrochronology age

Astronomy and Astrophysics

Volumn 515, Issue 11, 2010, Pages

  James, D J ^a,b   Barnes, S A ^c   Meibom, S ^d   Lockwood, G W ^c   Levine, S E ^e   Deliyannis, C ^f   Platais, I ^g   Steinhauer, A ^h   Hurley, B K ^a  

^a UNIVERSITY OF HAWAII AT HILO   (United States)

^b VANDERBILT UNIVERSITY   (United States)

^c LOWELL OBSERVATORY   (United States)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e US NAVAL OBSERVATORY   (United States)

^f INDIANA UNIVERSITY   (United States)

^g JOHNS HOPKINS UNIVERSITY   (United States)

^h STATE UNIVERSITY OF NEW YORK   (United States)

Author keywords

Globular clusters: individual: NGC 1039 (M 34); Methods: data analysis; Stars: fundamental parameters; Starspots

Indexed keywords

COLOR; DATA REDUCTION; GYROSCOPES; PHOTOMETERS; ROTATION; STARS; SURVEYS;

CLUSTER MEMBERSHIPS; COLOUR-MAGNITUDE DIAGRAMS; DIFFERENTIAL PHOTOMETRY; EMPIRICAL RELATIONS; GLOBULAR CLUSTERS: INDIVIDUAL; IN-BETWEEN; INDIANA; ISOCHRONES; LIGHT CURVES; METHODS:DATA ANALYSIS; OPEN CLUSTERS; PHOTOMETRIC VARIABLES; RADIAL VELOCITY; ROTATING STARS; ROTATION PERIOD; SOLAR TYPE STARS; STARS:FUNDAMENTAL PARAMETERS; STARSPOTS;

PHOTOMETRY;

EID: 77953632763     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913138     Document Type: Article

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