scholarly journals The Radio Continuum of the Large Magellanic Cloud. I. The Sources at 6 cm Wavelength

1972 ◽  
Vol 25 (5) ◽  
pp. 581 ◽  
Author(s):  
RX McGee ◽  
JW Brooks ◽  
RA Batchelor
Keyword(s):  
Radio Telescope ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Radio Continuum

The Large Magellanic Cloud has been surveyed in the radio continuum at a wavelength of 6 cm with the 4' are beam of the Parkes radio telescope. A catalogue of 95 sources and diagrams of their brightness contours are presented here.

scholarly journals The Radio Continuum of the Large Magellanic Cloud. II. Continuum Observations at 11 cm Wavelength

1972 ◽  
Vol 25 (5) ◽  
pp. 599 ◽  
Author(s):  
NW Broten
Keyword(s):  
Radio Telescope ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Magellanic Clouds ◽  
Radio Continuum ◽  
Half Power

Contour diagrams are presented for the radio continuum brightness of the Large and Small Magellanic Clouds observed at a wavelength of 11 cm. The observations were made with the Parkes 64 m radio telescope, whose half-power beamwidth was 7'�35 arc.

scholarly journals The Radio Continuum of the Large Magellanic Cloud. III. The Sources at 11 cm Wavelength

1972 ◽  
Vol 25 (5) ◽  
pp. 613 ◽  
Author(s):  
RX McGee ◽  
JW Brooks ◽  
RA Batchelor
Keyword(s):  
Radio Telescope ◽  
Large Magellanic Cloud ◽  
Low Noise ◽  
Magellanic Cloud ◽  
Radio Continuum ◽  
Noise Correlation ◽  
Radio Sources ◽  
Radio Brightness ◽  
Correlation Radiometer ◽  
30 Doradus

A catalogue is given of radio sources observed in the Large Magellanic Cloud at 11 cm wavelength. A map of the radio brightness in the 30 Doradus region is included. The observations were made with a low-noise correlation radiometer and the Parkes 64 m radio telescope.

scholarly journals Radio-continuum study of the supernova remnants in the large Magellanic Cloud: An SNR with a highly polarized breakout region: SNR J0455-6838

2008 ◽  
pp. 61-66 ◽  
Author(s):  
E.J. Crawford ◽  
M.D. Filipovic ◽  
Horta de ◽  
F.H. Stootman ◽  
J.L. Payne
Keyword(s):  
Supernova Remnants ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Radio Continuum ◽  
Strong Polarization ◽  
High Polarization ◽  
Moderate Resolution ◽  
Typical Appearance ◽  
D 43

We present the results of new moderate resolution ATCA observations of SNR J0455-6838. We found that this SNR exhibits a mostly typical appearance with rather steep and curved ?=-0.81?0.18 and D=43?31?1 pc. Regions of high polarization were detected, including unusually strong (~70%) region corresponding to the northern breakout. Such a strong polarization in breakout regions has not been observed in any other SNR.

scholarly journals An Australia Telescope Compact Array 20-cm radio continuum study of the Large Magellanic Cloud

2007 ◽  
Vol 382 (2) ◽  
pp. 543-552 ◽  
Author(s):  
A. Hughes ◽  
L. Staveley-Smith ◽  
S. Kim ◽  
M. Wolleben ◽  
M. Filipovic
Keyword(s):  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Radio Continuum ◽  
Compact Array

scholarly journals Magnetic Fields in the Irregular Galaxy LMC

1993 ◽  
Vol 157 ◽  
pp. 317-319
Author(s):  
Richard Wielebinski
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Radio Continuum ◽  
The South ◽  
Irregular Galaxy ◽  
New Radio ◽  
The Magnetic Field

New radio continuum surveys allowed the determination of the magnetic field in the Large Magellanic Cloud. The magnetic field is filamentary, extending to the south of the 30 Doradus nebula. Some possible explanations for this unusual morphology are discussed.

scholarly journals Multi-wavelength View of the Interstellar Medium in the Large Magellanic Cloud

1998 ◽  
Vol 15 (1) ◽  
pp. 136-140
Author(s):  
You-Hua Chu
Keyword(s):  
Interstellar Medium ◽  
Supernova Remnants ◽  
Optical Emission ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Radio Continuum ◽  
Emission Lines ◽  
X Rays ◽  
Multi Wavelength ◽  
The Relationship

AbstractThe Large Magellanic Cloud (LMC) has been surveyed in optical emission lines, X-rays, radio continuum, HI, and CO lines. These surveys provide views of the interstellar medium (ISM) in the LMC of unprecedented clarity, allowing us to study astrophysical processes and to examine the relationship among the different phases of the ISM. Multi-wavelength images are used to illustrate the physical structures of supernova remnants, superbubbles, and supergiant shells, as well as the global interstellar structure of the LMC.

scholarly journals Radio-continuum study of Large Magellanic Cloud supernova remnant J0509−6731

2014 ◽  
Vol 440 (4) ◽  
pp. 3220-3225 ◽  
Author(s):  
L. M. Bozzetto ◽  
M. D. Filipović ◽  
D. Urošević ◽  
R. Kothes ◽  
E. J. Crawford
Keyword(s):  
Supernova Remnant ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Radio Continuum

scholarly journals New 20-cm radio-continuum study of the small Magellanic cloud: Part I. Images

2011 ◽  
pp. 43-52 ◽  
Author(s):  
G.F. Wong ◽  
M.D. Filipovic ◽  
E.J. Crawford ◽  
Horta de ◽  
T. Galvin ◽  
...  
Keyword(s):  
Radio Telescope ◽  
High Sensitivity ◽  
Magellanic Cloud ◽  
Radio Continuum ◽  
Archival Data ◽  
Small Magellanic Cloud ◽  
Extended Structure ◽  
Future Studies ◽  
Compact Array

We present and discuss new high-sensitivity and resolution radiocontinuum images of the Small Magellanic Cloud (SMC) at ?=20 cm (?=1.4 GHz). The new images were created by merging 20-cm radio-continuum archival data, from the Australian Telescope Compact Array and the Parkes radio-telescope. Our images span from ?10"to ?150" in resolution and sensitivity of r.m.s.?0.5 mJy/beam. These images will be used in future studies of the SMC?s intrinsic sources and its overall extended structure.

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