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pro vyhledávání: '"Suryadi Siregar"'
Autor:
Suryadi Siregar
Publikováno v:
Journal of Mathematical and Fundamental Sciences, Vol 43, Iss 3 (2013)
Asteroid 1983 SA, well known as 3552 Don Quixote, is one of Near Earth Asteroids (NEAs) which is the most probable candidate for the cometary origin, or otherwise as Jupiter-Family-Comets (JFCs). The aim of this study is to investigate the possibilit
Externí odkaz:
https://doaj.org/article/6560e03258614d6ea956e87f163c74e7
Autor:
Suryadi Siregar, H. R. T. Wulandari, M. I. Arifyanto, Rhorom Priyatikanto, M. B. N. Kouwenhoven
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 457:1339-1351
Fragmentation and fission of giant molecular clouds occasionally results in a pair of gravitationally bound star clusters that orbit their mutual centre of mass for some time, under the influence of internal and external perturbations. We investigate
Publikováno v:
Journal of Physics: Conference Series. 1127:012053
Large Magellanic Cloud (LMC) has been known to host a significant fraction of binary star clusters whose dynamical and physical nature become interesting issue in accordance with the history of the galaxy. To understand the characteristics and the hi
Autor:
Suryadi Siregar
Publikováno v:
ITB Journal of Science, Vol 43, Iss 3, Pp 187-198 (2011)
Journal of Mathematical and Fundamental Sciences, Vol 43, Iss 3 (2013)
Journal of Mathematical and Fundamental Sciences, Vol 43, Iss 3 (2013)
Asteroid 1983 SA, well known as 3552 Don Quixote, is one of Near Earth Asteroids (NEAs) which is the most probable candidate for the cometary origin, or otherwise as Jupiter-Family-Comets (JFCs). The aim of this study is to investigate the possibilit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1035c579a6d034ecf3378342105294ea
http://arxiv.org/abs/1107.1024
http://arxiv.org/abs/1107.1024
Autor:
Suryadi Siregar
Publikováno v:
Publications of the Astronomical Society of Australia. 9:315-316
This paper briefly discusses the Aten, Apollo and Amor asteroid types (collectively referred to as AAAs), their perihelion distribution and orthogonal motion. There are 90 objects in these classes: 6 Atens, 46 Amors and 38 Apollos. The maximum distan
Autor:
Suryadi Siregar
Publikováno v:
Wide Components in Double and Multiple Stars ISBN: 9789401078429
This paper presents an overview on the software that will be used at the Bosscha Observatory of Indonesia for calculating the orbit and mass of visual binary system. The programme is based on the Thiele-van den Bos methods. The algorithm is designed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b7d8a7226012fabf7284c19bf97e0843
https://doi.org/10.1007/978-94-009-2987-6_39
https://doi.org/10.1007/978-94-009-2987-6_39
Publikováno v:
Journal of Physics: Conference Series; 2019, Vol. 1127 Issue 1, p1-1, 1p