Adding the s-Process Element Cerium to the APOGEE Survey: Identification and Characterization of Ce ii Lines in the H-band Spectral Window

Adding the s-Process Element Cerium to the APOGEE Survey: Identification and Characterization of Ce ii Lines in the H-band Spectral Window

Nine Ce II lines have been identified and characterized within the spectral window observed by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey (between lambda 1.51 and 1.69 mu m). At solar metallicities, cerium is an element that is produced predominantly as a result of th...

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Bibliographic Details
Main Authors: Cunha, Katia, Smith, Verne V., Hasselquist, Sten, Souto, Diogo, Shetrone, Matthew D., Allende Prieto, Carlos, Bizyaev, Dmitry, Frinchaboy, Peter, García-Hernández, D. Anibal, Holtzman, Jon, Johnson, Jennifer A., Jőnsson, Henrik, Majewski, Steven R., Mészáros, Szabolcs, Nidever, David, Pinsonneault, Mark, Schiavon, Ricardo P., Sobeck, Jennifer, Skrutskie, Michael F., Zamora, Olga, Zasowski, Gail, Fernández-Trincado, J. G.
Other Authors: Univ Arizona
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
stars: abundances
Online Access:http://hdl.handle.net/10150/625301
http://arizona.openrepository.com/arizona/handle/10150/625301

Internet

http://hdl.handle.net/10150/625301
http://arizona.openrepository.com/arizona/handle/10150/625301

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