Zobrazeno 1 - 10
of 12
pro vyhledávání: '"Majewski, Steven R."'
Autor:
McCormick, Caroline, Majewski, Steven R., Smith, Verne V., Hayes, Christian R., Cunha, Katia, Masseron, Thomas, Weiss, Achim, Shetrone, Matthew, Almeida, Andrés, Frinchaboy, Peter M., García-Hernández, Domingo Aníbal, Nitschelm, Christian
Standard stellar evolution theory poorly predicts the surface abundances of chemical species in low-mass, red giant branch (RGB) stars. Observations show an enhancement of p-p chain and CNO cycle products in red giant envelopes, which suggests the ex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ef9076982d0e49f18c46b977888fa51
http://arxiv.org/abs/2307.11191
http://arxiv.org/abs/2307.11191
Autor:
Muñoz, César, Monachesi, Antonela, Nidever, David L., Majewski, Steven R., Cheng, Xinlun, Olsen, Knut, Choi, Yumi, Zivick, Paul, Geisler, Douglas, Almeida, Andres, Muñoz, Ricardo R., Nitschelm, Christian, Roman-Lopes, Alexandre, Lane, Richard R., Fernández-Trincado, José G.
We present the first detailed chemical analysis from APOGEE-2S observations of stars in six regions of recently discovered substructures in the outskirts of the Magellanic Clouds (MCs) extending to 20 degrees from the Large MC (LMC) center. We also p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f5386398d5ba24a037d765a5ee50af7
http://arxiv.org/abs/2305.19460
http://arxiv.org/abs/2305.19460
Autor:
Wanderley, Fábio, Cunha, Katia, Souto, Diogo, Smith, Verne V., Cao, Lyra, Pinsonneault, Marc, Prieto, C. Allende, Covey, Kevin, Masseron, Thomas, Pascucci, Ilaria, Stassun, Keivan G., Terrien, Ryan, Bergsten, Galen J., Bizyaev, Dmitry, Fernández-Trincado, José G., Jönsson, Henrik, Hasselquist, Sten, Holtzman, Jon A., Lane, Richard R., Mahadevan, Suvrath, Majewski, Steven R., Minniti, Dante, Pan, Kaike, Serna, Javier, Sobeck, Jennifer, Stringfellow, Guy S.
We present a spectroscopic analysis of a sample of 48 M dwarf stars ($0.2 M_{\odot}< M < 0.6 M_{\odot}$) from the Hyades open cluster using high-resolution H-band spectra from the SDSS/APOGEE survey. Our methodology adopts spectrum synthesis with LTE
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6b9f8bc7d21e686091cdf3b6dd515cb9
http://arxiv.org/abs/2305.07065
http://arxiv.org/abs/2305.07065
Autor:
Kawata, Daisuke, Kawahara, Hajime, Gouda, Naoteru, Secrest, Nathan J., Kano, Ryouhei, Kataza, Hirokazu, Isobe, Naoki, Ohsawa, Ryou, Usui, Fumihiko, Yamada, Yoshiyuki, Graham, Alister W., Pettitt, Alex R., Asada, Hideki, Baba, Junichi, Bekki, Kenji, Dorland, Bryan N., Fujii, Michiko, Fukui, Akihiko, Hattori, Kohei, Hirano, Teruyuki, Kamizuka, Takafumi, Kashima, Shingo, Kawanaka, Norita, Kawashima, Yui, Klioner, Sergei A., Kodama, Takanori, Koshimoto, Naoki, Kotani, Takayuki, Kuzuhara, Masayuki, Levine, Stephen E., Majewski, Steven R., Masuda, Kento, Matsunaga, Noriyuki, Miyakawa, Kohei, Miyoshi, Makoko, Morihana, Kumiko, Nishi, Ryoichi, Notsu, Yuta, Omiya, Masashi, Sanders, Jason, Tanikawa, Ataru, Tsujimoto, Masahiro, Yano, Taihei, Aizawa, Masataka, Arimatsu, Ko, Biermann, Michael, Boehm, Celine, Chiba, Masashi, Debattista, Victor P., Gerhard, Ortwin, Hirabayashi, Masayuki, Hobbs, David, Ikenoue, Bungo, Izumiura, Hideyuki, Jordi, Carme, Kohara, Naoki, Löffler, Wolfgang, Luri, Xavier, Mase, Ichiro, Miglio, Andrea, Mitsuda, Kazuhisa, Newswander, Trent, Nishiyama, Shogo, Obuchi, Yoshiyuki, Ootsubo, Takafumi, Ouchi, Masami, Ozaki, Masanobu, Perryman, Michael, Prusti, Timo, Ramos, Pau, Read, Justin I., Rich, R. Michael, Schönrich, Ralph, Shikauchi, Minori, Shimizu, Risa, Suematsu, Yoshinori, Tada, Shotaro, Takahashi, Aoi, Tatekawa, Takayuki, Tatsumi, Daisuke, Tsujimoto, Takuji, Tsuzuki, Toshihiro, Urakawa, Seitaro, Uraguchi, Fumihiro, Utsunomiya, Shin, Van Eylen, Vincent, van Leeuwen, Floor, Wada, Takehiko, Walton, Nicholas A.
Japan Astrometry Satellite Mission for INfrared Exploration (JASMINE) is a planned M-class science space mission by the Institute of Space and Astronautical Science, the Japan Aerospace Exploration Agency. JASMINE has two main science goals. One is G
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::61cba55167431371e74735637c8736bf
Autor:
Beaton, Rachael L., Oelkers, Ryan J., Hayes, Christian R., Covey, Kevin R., Chojnowski, S. D., De Lee, Nathan, Sobeck, Jennifer S., Majewski, Steven R., Cohen, Roger, Fernandez-Trincado, Jose, Longa-Pena, Penelope, O'Connell, Julia E., Santana, Felipe A., Stringfellow, Guy S., Zasowski, Gail, Aerts, Conny, Anguiano, Borja, Bender, Chad, Canas, Caleb I., Cunha, Katia, Fleming, John Donor Scott W., Frinchaboy, Peter M., Feuillet, Diane, Harding, Paul, Hasselquist, Sten, Holtzman, Jon, Johnson, Jennifer A., Kollmeier, Juna A., Kounkel, Marina, Mahadevan, Suvrath, Price-Whelan, Adrian. M., Rojas-Arriagada, Alvaro, Roman-Zuniga, Carlos, Schlafly, Edward F., Schultheis, Mathias, Shetrone, Matthew, Simon, Joshua D., Stassun, Keivan G., Stutz, Amelia M., Tayar, Jamie, Teske, Johanna, Tkachenko, Andrew, Troup, Nick, Albareti, Franco D., Bizyaev, Dmitry, Bovy, Jo, Burgasser, Adam J., Comparat, Johan, Downes, Juan Jose, Geisler, Doug, Inno, Laura, Manchado, Arturo, Ness, Melissa K., Pinsonneault, Marc H., Prada, Francisco, Roman-Lopes, Alexandre, Simonian, Gregory V. A., Smith, Verne V., Yan, Renbin, Zamora, Olga
APOGEE-2 is a dual-hemisphere, near-infrared (NIR), spectroscopic survey with the goal of producing a chemo-dynamical mapping of the Milky Way Galaxy. The targeting for APOGEE-2 is complex and has evolved with time. In this paper, we present the upda
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a28064af193e7aac7619ab3bf94b961c
Autor:
Washington, Jasmin E., Lewis, Hannah M., Anguiano, Borja, Majewski, Steven R., Chojnowski, S. Drew, Smith, Verne V., Stassun, Keivan G., Prieto, Carlos Allende, Cunha, Katia, Nidever, David L., Garcia-Hernandez, D. A., Pan, Kaike
LIN 358 and SMC N73 are two symbiotic binaries in the halo of the Small Magellanic Cloud, each composed of a hot white dwarf accreting from a cool giant companion. In this work, we characterize these systems using a combination of SED-fitting to the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0576fbc938121f7a97a3d87bc996794a
Autor:
Skinner, Jacob, Covey, Kevin R., Bender, Chad F., Rivera, Noah, De Lee, Nathan, Souto, Diogo, Chojnowski, Drew, Troup, Nicholas, Badenes, Carles, Bizyaev, Dmitry, Blake, Cullen H., Burgasser, Adam, Canas, Caleb, Carlberg, Joleen, Chew, Yilen Gomez Maqueo, Deshpande, Rohit, Fleming, Scott W., Fernandez-Trincado, J. G., Garcia-Hernandez, D. A., Hearty, Fred, Kounkel, Marina, Longa-Pene, Penelope, Mahadevan, Suvrath, Majewski, Steven R., Minniti, Dante, Nidever, David, Oravetz, Audrey, Pan, Kaike, Stassun, Keivan, Terrien, Ryan, Zamora, Olga
Binary stars make up a significant portion of all stellar systems. Consequently, an understanding of the bulk properties of binary stars is necessary for a full picture of star formation. Binary surveys indicate that both multiplicity fraction and ty
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d4d9d8581868347c26296f63ca1c993a
Autor:
Povich, Matthew S., Smith, Nathan, Majewski, Steven R., Getman, Konstantin V., Townsley, Leisa K., Babler, Brian L., Broos, Patrick S., Indebetouw, R��my, Meade, Marilyn R., Robitaille, Thomas P., Stassun, Keivan G., Whitney, Barbara A., Yonekura, Yoshinori, Fukui, Yasuo
We present a catalog of 1439 young stellar objects (YSOs) spanning the 1.42 deg^2 field surveyed by the Chandra Carina Complex Project (CCCP), which includes the major ionizing clusters and the most active sites of ongoing star formation within the G
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::029e37d083d3eafc93a3c8a50527998e
http://arxiv.org/abs/1103.2060
http://arxiv.org/abs/1103.2060
Autor:
Frinchaboy, Peter M, Zasowski, Gail, Jackson, Kelly, Johnson, Jennifer A., Majewski, Steven R., Shetrone, Matthew, Rocha, Aaron
The Sloan Digital Sky Survey III/Apache Point Observatory Galactic Evolution Experiment (SDSS-III/APOGEE) is a large-scale spectroscopic survey of Galactic stars and star clusters. The SDSS-III/APOGEE survey is designed to produce high-S/N, R = 27,50
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::258ba77414698abc4f7693c350475e28
Autor:
Kalirai, Jason S., Beaton, Rachael L., Geha, Marla C., Gilbert, Karoline M., Guhathakurta, Puragra, Kirby, Evan N., Majewski, Steven R., Ostheimer, James C., Patterson, Richard J., Wolf, Joe
We present new Keck/DEIMOS spectroscopic observations of hundreds of individual stars along the sightline to Andromeda's first three discovered dwarf spheroidal galaxies (dSphs) - And I, II, and III, and leverage recent observations by our team of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f88678c814de6e55ff2c97965d48c224
http://arxiv.org/abs/0911.1998
http://arxiv.org/abs/0911.1998