Zobrazeno 1 - 10
of 51
pro vyhledávání: '"G. T. Birk"'
Publikováno v:
Astronomy & Astrophysics. 415:791-802
The formation and dynamical evolution of cometary plasma tails and magnetic boundary layers is studied by the first numerical plasma-neutral gas simulations. It is shown that collisional interaction between the cometary neutral envelope and the solar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cb96528e9ae7141a1c2336ff7809e260
https://doi.org/10.1051/0004-6361:20031695
https://doi.org/10.1051/0004-6361:20031695
Publikováno v:
Astrophysics and Space Science. 289:391-394
HI observations of high-velocity clouds (HVCs) indicate that they are interacting with their ambient medium. The question on the dynamical and thermal stabilization of a cold dense neutral cloud in a hot, thin, and magnetized ambient halo plasma is i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::06e334d60a3fdfd029142a5e32505d99
https://doi.org/10.1023/b:astr.0000014969.62388.15
https://doi.org/10.1023/b:astr.0000014969.62388.15
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 339:455-459
The remanent magnetization of meteorite material in the Solar system indicates that magnetic fields of several gauss are present in the protoplanetary disc. It is shown that such relatively strong magnetic fields can be generated in dusty protoplanet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bdbd1db3bc9996fce799771af0c71172
https://doi.org/10.1046/j.1365-8711.2003.06178.x
https://doi.org/10.1046/j.1365-8711.2003.06178.x
Publikováno v:
Journal of Plasma Physics. 66:213-222
The self-magnetisation of circumstellar disks is considered within an appropriate multifluid description. These disks are composed of ionised and neutral gas as well as of a charged dust component. The most important equation in this context is the g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2c5d2facc830604a7416d47af8d743f2
https://doi.org/10.1017/s0022377801001490
https://doi.org/10.1017/s0022377801001490
Publikováno v:
The Astrophysical Journal. 548:249-252
Observations show significant H\alpha-emissions in the Galactic halo near the edges of cold gas clouds of the Magellanic Stream. The source for the ionization of the cold gas is still a widely open question. In our paper we discuss the critical veloc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::072a380474d7e519251ab16e778a0a20
https://doi.org/10.1086/318690
https://doi.org/10.1086/318690
Publikováno v:
The Astrophysical Journal. 535:706-711
We report results of the most extensive and accurate monitoring yet undertaken for a supernova population in a starburst galaxy. The number of sources being monitored in M82's starburst nuclear region has been increased to 24, all of which now have d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7ab0ad4fd7b8d2859e325812198e8c58
https://doi.org/10.1086/308881
https://doi.org/10.1086/308881
Publikováno v:
Physics of Plasmas. 7:701-705
A self-consistent numerical model of self-generation and amplification of magnetic fields in weakly ionized protogalactic matter is presented. This model is based on three-dimensional two-fluid simulations of the dynamics expected for protogalactic p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e5f1b167b8f207eec213b705a5b9c2d1
https://doi.org/10.1063/1.873855
https://doi.org/10.1063/1.873855
Publikováno v:
The Astrophysical Journal. 518:177-182
Halos of active galaxies can show relatively strong magnetic fields. Observations indicate that such halo fields, which are significantly stronger than one would expect from the disk field strengths, seem to be associated with the dynamical flows and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3267c64a22b873db6d13ea4fb410c774
https://doi.org/10.1086/307273
https://doi.org/10.1086/307273
Publikováno v:
Physics of Plasmas. 5:3732-3736
Astrophysical plasmas typically have to be considered as highly collision-free from a kinetic point of view or highly ideal in a fluid description. This refers to near-Earth space plasmas, like the magnetosphere, or extragalactic objects like radio j
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0fcd629ae29e88b68baad7a027d04b1a
https://doi.org/10.1063/1.872983
https://doi.org/10.1063/1.872983
Publikováno v:
Computer Physics Communications. 112:7-22
The highly involved macroscopic low-frequency dynamics of partially ionized dusty plasmas can be studied by means of computational fluid simulations. We derived a general set of numerically tractable balance equations taking into account mass, moment
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3ce5c85ee410099487e8e5f988e734b9
https://doi.org/10.1016/s0010-4655(98)00044-7
https://doi.org/10.1016/s0010-4655(98)00044-7