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Autor:
Mack III, Claude E., Ge, Jian, Deshpande, Rohit, Wisniewski, John P., Stassun, Keivan G., Gaudi, B. Scott, Fleming, Scott W., Mahadevan, Suvrath, De Lee, Nathan, Eastman, Jason, Ghezzi, Luan, Hernandez, Jonay I. Gonzalez, Femenia, Bruno, Ferreira, Leticia, de Mello, Gustavo Porto, Crepp, Justin R., Sanchez, Daniel Mata, Agol, Eric, Beatty, Thomas G., Bizyaev, Dmitry, Brewington, Howard, Cargile, Phillip A., da Costa, Luiz N., Esposito, Massimiliano, Ebelke, Garret, Hebb, Leslie, Jiang, Peng, Kane, Stephen R., Lee, Brian, Maia, Marcio A. G., Malanushenko, Elena, Malanushenko, Victor, Oravetz, Daniel, Paegert, Martin, Pan, Kaike, Prieto, Carlos Allende, Peper, Joshua, Rebolo, Rafael, Roy, Arpita, Santiago, Basilio X., Schneider, Donald P., Simmons, Audrey, Siverd, Robert J., Snedden, Stephanie, Tofflemire, Benjamin M.
Publikováno v:
The Astronomical Journal, Volume 145, Issue 5, article id. 139, 15 pp. (2013)
We report the discovery of a highly eccentric, double-lined spectroscopic binary star system (TYC 3010-1494-1), comprising two solar-type stars that we had initially identified as a single star with a brown dwarf companion. At the moderate resolving
Externí odkaz:
http://arxiv.org/abs/1306.3157
