Silicon isotopic abundance toward evolved stars and its application for presolar grains
Artikel i vetenskaplig tidskrift, 2013
submillimeter: ISM
ISM: abundances
stars: late-type
ISM: molecules
Författare
T.-C. Peng
European Southern Observatory (ESO)
E. M. Humphreys
European Southern Observatory (ESO)
L. Testi
Ludwig-Maximilians-Universität München (LMU)
Osservatorio Astrofisico di Arcetri
European Southern Observatory (ESO)
A. Baudry
Laboratoire d'Astrophysique de Bordeaux
M. Wittkowski
European Southern Observatory (ESO)
M.G. Rawlings
National Radio Astronomy Observatory
I. de Gregorio-Monsalvo
European Southern Observatory (ESO)
Atacama Large Millimeter-submillimeter Array (ALMA)
Wouter Vlemmings
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
Lars-Åke Nyman
Atacama Large Millimeter-submillimeter Array (ALMA)
M.D. Gray
University of Manchester
C. De Breuck
European Southern Observatory (ESO)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 559 8-14 L8Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Fundament
Grundläggande vetenskaper
Infrastruktur
Onsala rymdobservatorium
DOI
10.1051/0004-6361/201322466