Zobrazeno 1 - 10
of 1 033
pro vyhledávání: '"Koppen J"'
Autor:
B.S. Hempenius-van Dijk
Publikováno v:
BMGN: Low Countries Historical Review, Vol 120, Iss 1, Pp 136-138 (2005)
Externí odkaz:
https://doaj.org/article/b2d6481dc8c84dd1999a546cbdae15ca
Autor:
L. van Poelgeest
Publikováno v:
BMGN: Low Countries Historical Review, Vol 105, Iss 1, Pp 119-121 (1990)
Externí odkaz:
https://doaj.org/article/b3ec34ffa5ae4a75871b1805085909c7
The removal of gas by ram pressure stripping of galaxies is treated by a purely kinematic description. The solution has two asymptotic limits: if the duration of the ram pressure pulse exceeds the period of vertical oscillations perpendicular to the
Externí odkaz:
http://arxiv.org/abs/1806.05887
Publikováno v:
Bijdragen en Mededelingen betreffende de Geschiedenis der Nederlanden. 120(1):136-138
Autor:
Hempenius-van Dijk, B.S.
Publikováno v:
Bijdragen en Mededelingen betreffende de Geschiedenis der Nederlanden, 120(1), 136-138. Koninklijk Nederlands Historisch Genootschap
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::aadb5384e07354a10911d9bd0b082263
https://research.rug.nl/en/publications/99cb64c6-91f8-44d6-a555-ced239c6cafc
https://research.rug.nl/en/publications/99cb64c6-91f8-44d6-a555-ced239c6cafc
Ram pressure stripping of galaxies in clusters can yield gas deficient disks. Previous numerical simulations based on various approaches suggested that, except for near edge-on disk orientations, the amount of stripping depends very little on the inc
Externí odkaz:
http://arxiv.org/abs/0904.3886
The influence of a time-varying ram pressure on spiral galaxies in clusters is explored with a new simulation method based on the N-body SPH/tree code GADGET. We have adapted the code to describe the interaction of two different gas phases, the diffu
Externí odkaz:
http://arxiv.org/abs/0706.3631
Aims: Chemical compositions and other properties of planetary nebulae around central stars of spectral types [WC], [WO], and wels are compared with those of `normal' central stars, in order to clarify the evolutionary status of each type and their in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611149
Autor:
L. van Poelgeest
Publikováno v:
BMGN: Low Countries Historical Review, Vol 105, Iss 1 (1990)
BMGN: Low Countries Historical Review, Vol 105, Iss 1, Pp 119-121 (1990)
BMGN: Low Countries Historical Review, Vol 105, Iss 1, Pp 119-121 (1990)
We compare abundances patterns in the Bulge for elements observed in stars and in planetary nebulae. Some alpha elements, like Mg and Ti, are overabundant respect to Fe, and others are not, like He, O, Si, S, Ar, Ca. The first ones favor a quick evol
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101215