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| Query : 2012MNRAS.427..393J |
2012MNRAS.427..393J - Mon. Not. R. Astron. Soc., 427, 393-396 (2012/November-3)
A possible influence of magnetic fields on the rotation of gas in NGC 253.
JALOCHA J., BRATEK L., PEKALA J. and KUTSCHERA M.
Abstract (from CDS):
The magnetic fields that are present in the galaxy NGC 253 are exceptionally strong. This means that they can influence the rotation of matter and hence the mass-to-light ratio. In this context, we address the issue of the presence of a non-baryonic dark matter halo in this galaxy.
Abstract Copyright: © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Journal keyword(s): galaxies: individual: NGC 253 - galaxies: kinematics and dynamics - galaxies: magnetic fields - galaxies: spiral - galaxies: structure
Errata: erratum vol. 441, p. 3502 (2014)
Simbad objects: 2
| Number of rows : 2 |
| 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 | NGC 253 | SyG | 00 47 33.134 | -25 17 19.68 | 8.03 | 6.94 | 8.1 | ~ | 3588 | 2 | ||
| 2 | NGC 891 | H2G | 02 22 32.907 | +42 20 53.95 | 11.08 | 10.81 | 9.93 | 7.86 | ~ | 1741 | 2 |
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