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이 학술지의 논문 검색
Combined Feedbacks of Magnetic Field and Radiative Transfer on Dense Core Collapse
Commercon, B.; Hennebelle, P.; Audit, E.; Chabrier, G.; Teyssier, R.; Henning, T. ASP; 1999 2012 p.13-18
Towards Understanding Simulated Feedback in AMR and SPH Codes and the Multi-Phase Nature of the ISM
Mitchell, N.L.; Bower, R.G.; Theuns, T.; Vorobyov, E.I. ASP; 1999 2012 p.19-24
Molecular Cloud Disruption and Chemical Enrichment of the ISM Caused by Massive Star Feedback
Fierlinger, K.M.; Burkert, A.; Diehl, R.; Dobbs, C.; Hartmann, D.H.; Krause, M.; Ntormousi, E.; Voss, R. ASP; 1999 2012 p.25-28
Importance of the Initial Conditions for Star Formation
Girichidis, P.; Federrath, C.; Banerjee, R.; Klessen, R. ASP; 1999 2012 p.29-32
Modeling Star-Forming Regions using a 3D Molecular Transport Code
Loughnane, R.M.; Redman, M.P.; Keto, E.R. ASP; 1999 2012 p.33-40
Binary Neutron Star Mergers Naturally Form Jets that can Power Short Gamma-Ray Bursts
Rezzolla, L. ASP; 1999 2012 p.41-50
Magnetic Field Generation During the Formation of the First Stars
Sur, S.; Federrath, C.; Schleicher, D.; Banerjee, R.; Klessen, R. ASP; 1999 2012 p.51-54
Numerical Simulations of Relativistic Magnetic Reconnection with Galerkin Methods
Zanotti, O.; Dumbser, M. ASP; 1999 2012 p.55-60
Numerical Simulations of Relativistic Magnetic Reconnection with Galerkin Methods
Zanotti, O.; Dumbser, M. San Francisco, Calif.; Astronomical Society of the Pacific 2012 p.55-218