National Astronomical Observatories, Chinese Academy of Sciences, No.20 Datun Road, Chaoyang District, 100101, Beijing, China Chenzhou Cui & Dongwei Fan Ministry of Education, Engineering Research Center for Integration and Application of E-Learning Technology, No.75 Fuxing Road, Haidian District, 10...
S. Chandrasekhar, Proceedings of the National Academy of Science 46, 253 (1960). DOI 10.1073/pnas.46.2.253 Google Scholar J.F. Hawley, C.F. Gammie, S.A. Balbus, Ap. J. 440, 742 (1995). DOI 10.1086/175311 Google Scholar A. Brandenburg, A. Nordlund, R.F. Stein, U. Torkelsso...
Evolutionary calculations of accreting protostars in the literature usually fall in one of two classes. In the constant accretion scenario, the accretion rate is kept at a constant level before dropping exponentially to reach the final mass. Constant accretion rates are predicted in semi-analytic mod...
As we show in Sect.3, the early measurement of the brightness evolution of kilonovae in the UV band will allow us to distinguish between different merger scenarios. However, the ability to distinguish between different models depends critically on the capability to point to the target location an...
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- 《Bulletin of the Russian Academy of Sciences Physics》 被引量: 1发表: 2008年 Weak Transitions Effect from First Excited States in Core of Massive Star in Pre-supernova Phase {document}nuclei (previously adopted in Dimarco et al., J. Phys. G Nucl. Part. Phys. 28 121 2002) of ...
D. I. Makarov (dim@sao.ru, Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Karachai-Cherkessia, Russia) N. V.Tyurina (tiurina@sai.msu.ru, Sternberg Astronomical Institute) Abstract We consider a thickness of stellar disks of late-type galaxies by analyzing the...
。InstituteofTheoreticalPhysics,ChineseAcademyofSciences,BeijinglOOOSO fReceived2September2oo2) Thec嬲 sectionofthedirectneutroncapturereaction C(n,,y)13C(1/2+)iscalculatedwiththeasymptotic nofmalizationcoe伍cientmethod.Theresultisingoodagreementwitharecentexperimentatlowenergy.An ...