Further evidence for vertical magnetic fields in the galaxy NGC 891

被引:14
作者
Scarrott, SM
Draper, PW
机构
[1] Physics Department, University of Durham, Durham DH1 3LE, South Road
关键词
polarization; galaxies; individual; NGC; 891; magnetic fields; spiral;
D O I
10.1093/mnras/278.2.519
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
An optical polarization map of NGC 891, an edge-on galaxy with similar properties to the Galaxy, confirms that there are vertical magnetic fields present in the bulge/halo above the inner part of the galactic disc. We find no evidence for large-scale magnetic fields in the central dust lane, or polarization created by scattering from dust grains within the dust lane and elsewhere in the galaxy.
引用
收藏
页码:519 / 524
页数:6
相关论文
共 25 条
[1]  
ALLEN RJ, 1978, ASTRON ASTROPHYS, V62, P397
[2]  
Berry D.S., 1985, THESIS U DURHAM
[3]   X-RAY-EMITTING GAS SURROUNDING THE SPIRAL GALAXY NGC-891 [J].
BREGMAN, JN ;
PILDIS, RA .
ASTROPHYSICAL JOURNAL, 1994, 420 (02) :570-575
[4]  
CHIBA M, 1994, ASTRON ASTROPHYS, V284, P731
[5]  
DAHLEM M, 1994, ASTRON ASTROPHYS, V290, P384
[6]   THE POLARIZATION OF STARLIGHT BY ALIGNED DUST GRAINS [J].
DAVIS, L ;
GREENSTEIN, JL .
ASTROPHYSICAL JOURNAL, 1951, 114 (02) :206-240
[7]  
DOLGINOV AZ, 1990, P IAU S, V140, P242
[8]  
DRAPER PW, 1988, THESIS U DURHAM
[9]  
GARCIABURILLO S, 1992, ASTRON ASTROPHYS, V266, P21
[10]  
GOLLA G, 1994, ASTRON ASTROPHYS, V284, P777