On a new parameter to estimate the helium content in old stellar systems

Publications of the Astronomical Society of the Pacific

Volumn 123, Issue 906, 2011, Pages 879-891

  Troisi, F ^a   Bono, G ^a,b   Stetson, P B ^c,d   Pietrinferni, A ^e   Weiss, A ^f   Fabrizio, M ^a   Ferraro, I ^a   di Cecco, A ^g   Iannicola, G ^b   Buonanno, R ^a,g   Calamida, A ^b   Caputo, F ^a,b   Corsi, C E ^b   Dall'Ora, M ^h   Kunder, A ⁱ   Monelli, M ^j   Nonino, M ^k   Piersimoni, A M ^e   Pulone, L ^b   Romaniello, M ^l   Walker, A R ⁱ   Zoccali, M ^m   more..

^a UNIVERSITY OF ROME TOR VERGATA   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^c NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^d University of Space Research Association   (United States)

^e INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

^f MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^g ITALIAN SPACE AGENCY   (Italy)

^h INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

ⁱ CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

^j INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^k INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^l EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^m PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

more..

Author keywords

[No Author keywords available]

Indexed keywords

EID: 80051644509     PISSN: 00046280     EISSN: None     Source Type: Journal    
DOI: 10.1086/661534     Document Type: Article

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