Peculiarities of simulation of thin flat discs with central objects in accordance with their spatial location-Reference-Cited by-同舟云学术

Peculiarities of simulation of thin flat discs with central objects in accordance with their spatial location

Published:2011-06 Issue:3 Volume:27 Page:140-153
ISSN:0884-5913
Container-title:Kinematics and Physics of Celestial Bodies
language:en
Short-container-title:Kinemat. Phys. Celest. Bodies

Author:

Zakhozhay V. A.,Zakhozhay O. V.,Vidmachenko A. P.

Publisher

Allerton Press

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.3103/S0884591311030068.pdf

Reference14 articles.

1. V. A. Zakhozhay, “Problem of Planetary Systems Existence. II. Expected Properties and First Search Results,” Visn. Astron. Shkoli 4(2), 55–72 (2005).

2. I. A. Zakhozhay and O. V. Zakhozhay, “Disks Around the Nearest Stars and Substars,” Kinem. Fiz. Nebes. Tel 26(1), 3–30 (2010) [Kinem. Phys. Celest. Bodies 26, 1 (2010)].

3. A. I. Pisarenko, A. A. Yatsenko, and V. A. Zakhozhai, “Evolution Model for Substellar Objects,” Astron. Zh. 84(8), 675–684 (2007) [Astron. Rep. 51, 605 (2007)].

4. V. S. Safronov, Evolution of the Protoplanetary Cloud and the Formation of the Earth and Planets (Nauka, Moscow, 1969; Israel Program for Scientific Translations, Jerusalem, 1972).

5. P. J. Armitage, “Lecture Notes on the Formation and Early Evolution of Planetary Systems,” arXiv: astro-ph/0701485v1 (2007).

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