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Results 1 - 10 of about 30181. Search took: 0.91 seconds.
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Feasibility Study for a Plasma Dynamo Facility to Investigate Fundamental Processes in Plasma Astrophysics. Final report
by Forest, Cary B.; University of Wisconsin, Madison, WI (United States). Funding organisation: USDOE Office of Science, Office of Fusion Energy Sciences (United States)
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EARLY-STAGE MASSIVE STAR FORMATION NEAR THE GALACTIC CENTER: Sgr C
http://dx.doi.org/10.1088/2041-8205/775/2/L50
by Kendrew, S.; Johnston, K.; Beuther, H. (Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg (Germany)); Ginsburg, A.; Bally, J.; Battersby, C. (CASA, University of Colorado at Boulder, UCB 389, Boulder, CO 80309 (United States)); Cyganowski, C. J. (Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States)), E-mail: kendrew@mpia.de
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α-α interaction reexamined in the context of the Sao Paulo potential: possible applications in astrophysics?
by Gasques, L.R.; Chamon, L.C.; Botero, D.F.M. (Universidade de Sao Paulo (DFN/USP), SP (Brazil). Dept. de Fisica Nuclear); Alves, L.F.M. (Instituto Federal de Educacao, Ciencia e Tecnologia (Brazil)); Carlson, B.V. (Instituto Tecnologico de Aeronautica (CTA/ITA), Sao Jose dos Campos, SP (Brazil). Dept. de Fisica Nuclear); Rossi Junior, E.S. (Centro Universitario FIEO(UNIFIEO), SP (Brazil)); Sociedade Brasileira de Fisica, Sao Paulo, SP (Brazil)
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CENTAURUS A AS A POINT SOURCE OF ULTRAHIGH ENERGY COSMIC RAYS
http://dx.doi.org/10.1088/0004-637X/764/2/121
by Kim, Hang Bae (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seoul 133-791 (Korea, Republic of)), E-mail: hbkim@hanyang.ac.kr
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INFRARED OBSERVATIONS OF THE MILLISECOND PULSAR BINARY J1023+0038: EVIDENCE FOR THE SHORT-TERM NATURE OF ITS INTERACTING PHASE IN 2000-2001
http://dx.doi.org/10.1088/0004-637X/764/2/144
by Wang, Xuebing; Wang, Zhongxiang (Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030 (China)); Morrell, Nidia (Las Campanas Observatory, Observatories of the Carnegie Institution of Washington, La Serena (Chile))
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Scale-Covariant Theory of Gravitation Through Self-Similarity
http://dx.doi.org/10.1088/0256-307X/29/5/050401
by Belinchón José Antonio (Department of Nuclear, Molecular and Atomic Physics, University Complutense of Madrid, E-28040 (Spain)), E-mail: abelcal@ciccp.es
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HARD X-RAY LAGS IN ACTIVE GALACTIC NUCLEI: TESTING THE DISTANT REVERBERATION HYPOTHESIS WITH NGC 6814
http://dx.doi.org/10.1088/2041-8205/777/2/L23
by Walton, D. J.; Harrison, F. A. (Cahill Centre for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States)); Zoghbi, A.; Reynolds, C. S. (Department of Astronomy, University of Maryland, College Park, MD 20742 (United States)); Cackett, E. M. (Department of Physics and Astronomy, Wayne State University, Detroit, MI 48201 (United States)); Uttley, P. (Astronomical Institute Anton Pannekoek, University of Amsterdam, Postbus 94249, NL-1090 GE Amsterdam (Netherlands)); Fabian, A. C.; Kara, E. (Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA (United Kingdom)); Miller, J. M.; Reis, R. C. (Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109 (United States))
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ON THE GRAVITATIONAL FIELDS OF MACLAURIN SPHEROID MODELS OF ROTATING FLUID PLANETS
http://dx.doi.org/10.1088/0004-637X/764/1/67
by Kong, Dali; Zhang, Keke (Center for Geophysical and Astrophysical Fluid Dynamics and Department of Mathematical Sciences, University of Exeter, Exeter EX4 4QF (United Kingdom)); Schubert, Gerald (Department of Earth and Space Sciences and Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA (United States)), E-mail: D.Kong@exeter.ac.uk, E-mail: kzhang@ex.ac.uk, E-mail: schubert@ucla.edu
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A New Solution to Einstein's Field Equations
http://dx.doi.org/10.1088/0256-307X/26/6/060401
by Ming, Shen (Center of Mathematical Sciences, Zhejiang University, Hangzhou 310027 (China)), E-mail: shenming0516@163.com
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