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Date: 2014
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/326400
Description: A new set of very high signal-to-noise (S/N > 100/1), medium-resolution (R ~ 3000) optical spectra have been obtained for 302 of the candidate "weak-metal" stars selected by Bidelman & MacConnell. We ... More
Full Text: Full Text
Reviewed: Reviewed
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/212788
Description: Carbon-enhanced metal-poor (CEMP) stars in the halo components of the Milky Way are explored, based on accurate determinations of the carbon-to-iron ([C/Fe]) abundance ratios and kinematic quantities ... More
Reviewed: Reviewed
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/171049
Description: Carollo et al. have recently resolved the stellar population of the Milky Way halo into at least two distinct components, an inner halo and an outer halo. This result has been criticized by Schönrich ... More
Reviewed: Reviewed
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/213716
Description: The structure and kinematics of the recognized stellar components of the Milky Way are explored, based on well-determined atmospheric parameters and kinematic quantities for 32360 "calibration stars" ... More
Reviewed: Reviewed
Authors: Yanny, Brian | Rockosi, Constance M | Newberg, Heidi Jo | Knapp, Gillian R | Adelman-Mccarthy, Jennifer K | Alcorn, Bonnie | Allam, Sahar S | Allende-Prieto, Carlos | An, Doekkeun | Anderson, Kurt S. J | Anderson, Scott F | Bailer-Jones, Coryn A L | Bastian, Steven | Beers, Timothy C | Bell, Eric F | Belokurov, Vasily | Bizyaev, Dmitriy V | Blythe, Norman | Bochanski, John J | Boroski, William N | Brinchmann, Jarle | Brinkmann, Jonathan O. N | Brewington, Howard J | Carey, Larry N | Cudworth, Kyle M | Evans, Michael L | Evans, N. W | Gates, Evalyn I | Gänsicke, Boris T | Gillespie, Bruce A | Gilmoure, Gerald | Nebot Gomez-Moran, Ada | Grebel, Eva K | Greenwell, Jim | Gunn, James E | Jordan, Cathy | Jordan, Wendell | Harding, Paul | Harris, Hugh C | Hendry, John S | Holder, Diana | Ivans, Inese I | Ivezic, Zeljko | Jester, Sebastian | Johnson, Jennifer | Kent, Stephen M | Kleinman, Scot J | Kniazev, Alexei Yu | Krzesinski, Jurek | Kron, Richard G | Kuropatkin, Nikolay | Lebedeva, Svetlana | Lee, Young Sun | Leger, R. French | Lepine, Sebastien | Levine, Stephen | Lin, Huan | Long, Dan C | Loomis, Craig P | Lupton, Robert H | Malanushenko, Olena | Malanushenko, Viktor | Margon, Bruce | Martinez-Delgado, David | McGehee, Peregrine M | Monet, David | Morrison, Heather L | Munn, Jeffrey A | Nielsen, Eric H | Nitta, Atsuko | Norris, John E | Oravetz, Daniel J | Owen, Russell E | Padmanabhan, Nikhil | Pan, Kaike | Peterson, R. S | Pier, Jeffrey R | Platson, Jared | Re Fiorentin, P | Richards, Gordan T | Rix, Hans-Walter | Schlegel, David J | Schneider, Donald P | Schreiber, Matthias R | Schwope, Axel D | Sibley, Valena C | Simmons, Audrey E | Snedden, Stephanie A | Smith, J. Allyn | Stark, Larry | Stauffer, Fritz | Steinmetz, Matthias | S toughton, Christopher | SubbaRao, Mark U | Szkody, Paula | Szalay, Alex S | Thakar, Aniruddha | Thirupathi, Sivarani | Tucker, Douglas L | Uomoto, Alan K | Vanden Berk, Daniel E | Vidrih, Simon | Wadadekar, Yogesh | Watters, Shannon | Wilhelm, Ron | Wyse, Rosemary F. G | Yarger, Jean | Zucker, Daniel Benjamin
Date: 2009
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/1147327
Description: 23 page(s)
Reviewed: Reviewed
Date: 2008
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/216134
Description: The chemical compositions of seven CEMP turnoff stars are determined from high-resolution spectroscopy. Five are selected from the SDSS SEGUE sample of metal-poor stars. Another star chosen from the S ... More
Reviewed: Reviewed
Date: 2007
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/216044
Description: The halo of the Milky Way provides unique elemental abundance and kinematic information on the first objects to form in the Universe, and this information can be used to tightly constrain models of ga ... More
Reviewed: Reviewed
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