SCOPUS 정보 검색 플랫폼

Volumn T133, Issue , 2008, Pages

A new sample of extremely/ultra metal-poor stars

(14) Garcia Perez A E a Christlieb, N b Ryan, S G a Beers, T C c Aoki, W d Asplund, M e Barklem, P S f Bessell, M S g Eriksson, K f Frebel, A h Gustafsson, B f Korn, A J f Nordstrom B i Norris, J E g

a UNIVERSITY OF HERTFORDSHIRE (United Kingdom)

b UNIVERSITÄT HEIDELBERG (Germany)

c MICHIGAN STATE UNIVERSITY (United States)

d NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN (Japan)

e MAX PLANCK INSTITUT FÜR ASTROPHYSIK (Germany)

f UPPSALA UNIVERSITY (Sweden)

g AUSTRALIAN NATIONAL UNIVERSITY (Australia)

h The University of Texas at Austin (United States)

i UNIVERSITY OF COPENHAGEN (Denmark)

Author keywords

[No Author keywords available]

Indexed keywords

ECHELLE SPECTROGRAPH; EFFECTIVE TEMPERATURE; EUROPEAN SOUTHERN OBSERVATORY; FOUR-ORDER; HIGH SPECTRAL RESOLUTION; HYDROGEN LINES; IRON CONTENT; ISOCHRONES; METAL-POOR STAR; METALLICITIES; NEUTRAL LITHIUM; SUBGIANTS; VERY LARGE TELESCOPE;

LITHIUM; OPTICAL TELESCOPES;

STARS;

EID: 70350654387 PISSN: 02811847 EISSN: None Source Type: Conference Proceeding
DOI: 10.1088/0031-8949/2008/T133/014036 Document Type: Conference Paper

Times cited : (8)

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