Chemically tagging the Hyades stream: Does it partly originate from the Hyades cluster?

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 2, 2011, Pages 1138-1154

  Pompeia L ^a,b   Masseron, T ^a   Famaey, B ^c,d   van Eck, S ^a   Jorissen, A ^a   Minchev, I ^e   Siebert, A ^c   Sneden, C ^f   Lepine J R D ^g   Siopis, C ^a   Gentile, G ^a,h   Dermine, T ^a   Pasquato, E ^a   van Winckel, H ⁱ   Waelkens, C ⁱ   Raskin, G ⁱ   Prins, S ⁱ   Pessemier, W ⁱ   Hensberge, H ^j   Fremat Y ^j   Dumortier, L ^j   Bienayme O ^c   more..

^a UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

^b INSTITUTO DE PESQUISA E DESENVOLVIMENTO   (Brazil)

^c UNIVERSITÉ DE STRASBOURG   (France)

^d UNIVERSITY OF BONN   (Germany)

^e ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^f UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^g UNIVERSITY OF SÃO PAULO   (Brazil)

^h GHENT UNIVERSITY   (Belgium)

ⁱ UNIVERSITY OF LEUVEN   (Belgium)

^j ROYAL OBSERVATORY OF BELGIUM   (Belgium)

more..

Author keywords

Galaxy: evolution; Galaxy: kinematics and dynamics; Open clusters and associations: individual: Hyades

Indexed keywords

ASTROPHYSICS; CHEMICAL ANALYSIS; GALAXIES; GEOMETRICAL OPTICS; METALS;

ACTION SPACES; CHEMICAL TAGS; ELEMENT ABUNDANCES; GALAXIES: KINEMATICS AND DYNAMICS; GALAXY EVOLUTION; MASS FUNCTIONS; METALLICITIES; OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: HYADES; RANDOM SAMPLE; SPACE DISTRIBUTION;

STARS;

EID: 79960615010     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18685.x     Document Type: Article

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