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Results 1 - 10 of about 36726. Search took: 1.36 seconds.
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A modern search for Wolf-Rayet stars in the Magellanic Clouds: First results
http://dx.doi.org/10.1088/0004-637X/788/1/83
by Massey, Philip; Neugent, Kathryn F. (Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001 (United States)); Morrell, Nidia (Las Campanas Observatory, Carnegie Observatories, Casilla 601 La Serena (Chile)); Hillier, D. John (Department of Physics and Astronomy and Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT PACC), University of Pittsburgh, Pittsburgh, PA 15260 (United States)), E-mail: phil.massey@lowell.edu, E-mail: kneugent@lowell.edu, E-mail: nmorrell@lco.cl, E-mail: hillier@pitt.edu
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Dynamical evolution of viscous disks around be stars. II. Polarimetry
http://dx.doi.org/10.1088/0004-637X/785/1/12
by Haubois, X. (LESIA, Observatoire de Paris, CNRS UMR 8109, UPMC, Université Paris Diderot, 5 place Jules Janssen, F-92195 Meudon (France)); Mota, B. C.; Carciofi, A. C.; Bednarski, D. (Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão 1226, Cidade Universitária, São Paulo, SP 05508-090 (Brazil)); Draper, Z. H. (Department of Physics and Astronomy, University of Victoria, 3800 Finnerty Road, Victoria, BC V8P 5C2 (Canada)); Wisniewski, J. P. (H. L. Dodge Department of Physics and Astronomy, University of Oklahoma, 440 West Brooks St Norman, OK 73019 (United States)); Rivinius, Th. (European Organisation for Astronomical Research in the Southern Hemisphere, Casilla 19001, Santiago 19 (Chile)), E-mail: xavier.haubois@obspm.fr
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Stochastic modeling of the Fermi/LAT γ-ray blazar variability
http://dx.doi.org/10.1088/0004-637X/786/2/143
by Sobolewska, M. A.; Siemiginowska, A. (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)); Kelly, B. C. (Department of Physics, Broida Hall, University of California, Santa Barbara, CA 93107 (United States)); Nalewajko, K. (JILA, University of Colorado and National Institute of Standards and Technology, 440 UCB, Boulder, CO 80309 (United States)), E-mail: malgosia@camk.edu.pl
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Seven new carbon-enhanced metal-poor RR Lyrae stars
http://dx.doi.org/10.1088/0004-637X/787/1/6
by Kennedy, Catherine R.; Stancliffe, Richard J. (Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611 (Australia)); Kuehn, Charles (Sydney Institute for Astronomy, University of Sydney, Sydney, NSW 2006 (Australia)); Beers, Timothy C.; Kinman, T. D. (National Optical Astronomy Observatory, Tucson, AZ 85719 (United States)); Placco, Vinicius M. (Gemini Observatory, Hilo, HI 96720 (United States)); Reggiani, Henrique; Rossi, Silvia (Departamento de Astronomia, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, São Paulo, SP 05508-900 (Brazil)); Lee, Young Sun (Department of Astronomy, New Mexico State University, Las Cruces, NM 88003 (United States)), E-mail: catherine.kennedy@anu.edu.au
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Dependence of the outer density profiles of halos on their mass accretion rate
http://dx.doi.org/10.1088/0004-637X/789/1/1
by Diemer, Benedikt; Kravtsov, Andrey V. (Department of Astronomy and Astrophysics, The University of Chicago, Chicago, IL 60637 (United States)), E-mail: bdiemer@oddjob.uchicago.edu
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A new optical survey of supernova remnant candidates in M31
http://dx.doi.org/10.1088/0004-637X/786/2/130
by Lee, Jong Hwan; Lee, Myung Gyoon (Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul 151-747 (Korea, Republic of)), E-mail: leejh@astro.snu.ac.kr, E-mail: mglee@astro.snu.ac.kr
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Outflow and hot dust emission in broad absorption line quasars
http://dx.doi.org/10.1088/0004-637X/786/1/42
by Zhang, Shaohua; Zhou, Hongyan (Polar Research Institute of China, 451 Jinqiao Road, Shanghai 200136 (China)); Wang, Huiyuan; Wang, Tinggui; Xing, Feijun; Jiang, Peng (Key Laboratory for Research in Galaxies and Cosmology, University of Science and Technology of China, Chinese Academy of Sciences, Hefei, Anhui 230026 (China)); Zhang, Kai (Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030 (China)), E-mail: zhangshaohua@pric.gov.cn, E-mail: whywang@mail.ustc.edu.cn
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Evolution of the fraction of clumpy galaxies at 0.2 < z < 1.0 in the cosmos field
http://dx.doi.org/10.1088/0004-637X/786/1/15
by Murata, K. L. (Department of Particle and Astrophysical Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602 (Japan)); Kajisawa, M. (Graduate School of Science and Engineering, Ehime University, Bunkyo-cho, Matsuyama 790-8577 (Japan)); Taniguchi, Y.; Kobayashi, M. A. R.; Shioya, Y. (Research Center for Space and Cosmic Evolution, Ehime University, Bunkyo-cho, Matsuyama 790-8577 (Japan)); Capak, P. (Spitzer Science Center, 314-6 Caltech, Pasadena, CA 91125 (United States)); Ilbert, O. (Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille), UMR 7326, F-13388 Marseille (France)); Koekemoer, A. M. (Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)); Salvato, M. (Max Planck Institut für Plasma Physik and Excellence Cluster, D-85748 Garching (Germany)); Scoville, N. Z. (California Institute of Technology, MC 249-17, 1200 East California Boulevard, Pasadena, CA 91125 (United States)), E-mail: murata.katsuhiro@g.mbox.nagoya-u.ac.jp
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High-resolution ultraviolet radiation fields of classical T Tauri stars
http://dx.doi.org/10.1088/0004-637X/784/2/127
by France, Kevin (Center for Astrophysics and Space Astronomy, University of Colorado, 389 UCB, Boulder, CO 80309 (United States)); Schindhelm, Eric (Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302 (United States)); Bergin, Edwin A. (Department of Astronomy, University of Michigan, 830 Dennison Building, 500 Church Street, Ann Arbor, MI 48109 (United States)); Roueff, Evelyne; Abgrall, Hervé (LERMA and UMR 8112 du CNRS, Observatoire de Paris, Section de Meudon, Place J. Janssen, F-92195 Meudon (France)), E-mail: kevin.france@colorado.edu
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On the variation of solar flare coronal X-ray source sizes with energy
http://dx.doi.org/10.1088/0004-637X/787/1/86
by Jeffrey, Natasha L. S.; Kontar, Eduard P.; Bian, Nicolas H. (School of Physics and Astronomy, University of Glasgow, G12 8QQ Glasgow (United Kingdom)); Emslie, A. Gordon (Department of Physics and Astronomy, Western Kentucky University, Bowling Green, KY 42101 (United States)), E-mail: n.jeffrey@physics.gla.ac.uk
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