30.9 MHz observations of the radio halo in the coma cluster of galaxies

1989 ◽  
Vol 97 ◽  
pp. 1561 ◽  
Author(s):  
Patricia A. Henning
Keyword(s):  
Coma Cluster ◽  
Radio Halo ◽  
Cluster Of Galaxies

On the origin of the radio halo in the coma cluster of galaxies

1990 ◽  
Vol 105 (8-9) ◽  
pp. 845-856
Author(s):  
Kwang-Tae Kim
Keyword(s):  
Coma Cluster ◽  
Radio Halo ◽  
Cluster Of Galaxies

scholarly journals The Strength and Structure of the Intracluster Magnetic Field in the Coma Cluster of Galaxies

1990 ◽  
Vol 140 ◽  
pp. 483-485
Author(s):  
K.-T. Kim ◽  
P. P. Kronberg
Keyword(s):  
Magnetic Field ◽  
Dynamic Range ◽  
High Dynamic Range ◽  
Coma Cluster ◽  
Radio Halo ◽  
Cluster Of Galaxies ◽  
Probe Experiment ◽  
High Dynamic ◽  
Intracluster Gas ◽  
Gas Component

A new series of detailed observations of the Coma cluster of galaxies has been undertaken with the aim of better specifying the intracluster gas component throgh high dynamic range, combined-telescope observations of the radio halo emission from the cluster which detect both the cluster-scale and galaxy-scale emission. By combining these multi-frequency maps with a Faraday rotation probe experiment using cluster and background sources, and the published X-ray data, we have been able to estimate the intracluster magnetic field strength independently of the unusal assumption of equipartition. The result is approximately 2 microgauss and the tangling of the rms field occurs on an optical galaxy scale.

Deep low frequency image of Coma cluster of galaxies

2019 ◽  
Author(s):  
Dharam V Lal ◽  
C.H. Ishwara-Chandra
Keyword(s):  
Low Frequency ◽  
Coma Cluster ◽  
Cluster Of Galaxies

On the Structure of the Coma Cluster of Galaxies

1984 ◽  
Vol 305 (4) ◽  
pp. 175-185 ◽  
Author(s):  
F. W. Baier
Keyword(s):  
Coma Cluster ◽  
Cluster Of Galaxies

scholarly journals A deep wide survey of faint low surface brightness galaxies in the direction of the Coma cluster of galaxies

2006 ◽  
Vol 459 (3) ◽  
pp. 679-692 ◽  
Author(s):  
C. Adami ◽  
R. Scheidegger ◽  
M. Ulmer ◽  
F. Durret ◽  
A. Mazure ◽  
...  
Keyword(s):  
Surface Brightness ◽  
Coma Cluster ◽  
Cluster Of Galaxies ◽  
Low Surface Brightness ◽  
Low Surface Brightness Galaxies

A new stellar standard sequence in the coma cluster of galaxies. (preliminary report)

1978 ◽  
Vol 299 (3) ◽  
pp. 117-120 ◽  
Author(s):  
F. Börngen ◽  
N. Richter
Keyword(s):  
Preliminary Report ◽  
Coma Cluster ◽  
Standard Sequence ◽  
Cluster Of Galaxies

High-sensitivity radio observations of the Coma cluster of galaxies

1990 ◽  
Vol 99 ◽  
pp. 1381 ◽  
Author(s):  
T. Venturi ◽  
G. Giovannini ◽  
L. Feretti
Keyword(s):  
High Sensitivity ◽  
Coma Cluster ◽  
Radio Observations ◽  
Cluster Of Galaxies

The halo and magnetic field of the Coma cluster of galaxies

1990 ◽  
Vol 355 ◽  
pp. 29 ◽  
Author(s):  
K.-T. Kim ◽  
P. P. Kronberg ◽  
P. E. Dewdney ◽  
T. L. Landecker
Keyword(s):  
Magnetic Field ◽  
Coma Cluster ◽  
Cluster Of Galaxies

scholarly journals Ubiquitous ram pressure stripping in the Coma cluster of galaxies

2018 ◽  
Vol 618 ◽  
pp. A130 ◽  
Author(s):  
G. Gavazzi ◽  
G. Consolandi ◽  
M. L. Gutierrez ◽  
A. Boselli ◽  
M. Yoshida
Keyword(s):  
Coma Cluster ◽  
Ionized Gas ◽  
San Pedro ◽  
Cluster Of Galaxies ◽  
Irregular Galaxies ◽  
Ram Pressure ◽  
Extended Component ◽  
Galaxy Population ◽  
Early Type Galaxy ◽  
Kinematic Properties

We report the detection of Hα trails behind three new intermediate-mass irregular galaxies in the NW outskirts of the nearby cluster of galaxies Abell 1656 (Coma). Hints that these galaxies possess an extended component were found in earlier, deeper Hα observations carried out with the Subaru telescope. However the lack of a simultaneous r-band exposure, together with the presence of strong stellar ghosts in the Subaru images, prevented us from quantifying the detections. We therefore devoted one full night of Hα observation to each of the three galaxies using the San Pedro Martir 2.1 m telescope. One-sided tails of Hα emission of 10–20 kpc projected size were detected, suggesting an ongoing ram pressure stripping event. We added these 3 new sources of extended ionized gas to the 12 previously found, NGC 4848, and NGC 4921 whose ram pressure stripping is certified by HI asymmetry. This brings the number sources with Hα trails to 17 gaseous tails out of 27 (63%) late-type galaxies (LTG) members of the Coma cluster with direct evidence of ram pressure stripping. The 27 LTG galaxies, among these the 17 with extended Hα tails, have kinematic properties that are different from the rest of the early-type galaxy population of the core of the Coma cluster, as they deviate in the phase-space diagram |ΔV|/σ versus r/R200.

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