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| Query : 1994A&A...286L..13K |
1994A&A...286L..13K - Astronomy and Astrophysics, volume 286L13-16 (1994/6-1)
The impact of a high velocity cloud onto the galactic disk.
KERP J., LESCH H. and MACK K.-H.
Abstract (from CDS):
We present ROSAT and radio observations of a high velocity cloud (HVC) which encounters the Milky Way. At the edges of the HVC90.5+42.5-130 X-ray emitting gas (with Te~=2.106K) as well as relativistic electrons and magnetic fields (traced by non-thermal radio continuum emission) exist. We propose that the kinetic energy of the HVC is effectively transferred into heat via magnetic drag. The field lines are compressed, turbulently mixed and dissipated via magnetic reconnection, i.e. electric currents.
Abstract Copyright: ∼
Journal keyword(s): Galaxy: halo - MHD - radio continuum: ISM - X-ray: general - X-ray: ISM
Simbad objects: 4
| Number of rows : 4 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | LEDA 2817000 | G | 16 12 24.5970948624 | +59 46 10.371674676 | ~ | 7 | 0 | |||||
| 2 | HVC 090.5+42.5-130 | HVC | 16 15 52.8 | +59 42 00 | ~ | 3 | 0 | |||||
| 3 | NAME HVC Complex C | HVC | 16 34.8 | +63 07 | ~ | 273 | 1 | |||||
| 4 | NAME Draco Cloud | MoC | 16 48 17 | +60 11.8 | ~ | 77 | 1 |
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