Radio Continuum Observations of the Magellanic Clouds

Author(s):  
D. S. Mathewson
1999 ◽  
Vol 192 ◽  
pp. 104-107
Author(s):  
M.D. Filipović ◽  
W. Pietsch ◽  
G. L. White ◽  
F. Haberl ◽  
L. Staveley-Smith ◽  
...  

We present our high-resolution radio-continuum and X-ray study of supernova remnants (SNRs) in the Magellanic Clouds (MCs). These investigations are based on Australia Telescope Compact Array (ATCA) radio-continuum and ROSAT X-ray observations. Our main aim is to study a complete sample of the MC SNRs and H II regions.


2011 ◽  
Vol 7 (S283) ◽  
pp. 334-335 ◽  
Author(s):  
Evan J. Crawford ◽  
Miroslav D. Filipović ◽  
Ivan S. Bojičić ◽  
Martin Cohen ◽  
Jeff L. Payne ◽  
...  

AbstractWe present preliminary results of our deep Australia Telescope Compact Array (ATCA) radio-continuum survey of the Magellanic Clouds Planetary Nebulae.


1978 ◽  
Vol 77 ◽  
pp. 131-137
Author(s):  
J.B. Whiteoak

The observation in 1965 of absorption due to the 18 cm ground-state transition of OH in the direction of Cas A (Weinreb et al., 1963) marked the first occasion on which a molecular cloud was detected at radio wavelengths. However, it was not until the later discovery of high-intensity OH emission (Weaver et al., 1965) that attention turned to nearby galaxies. Unfortunately, searches for OH emission in the Magellanic Clouds (McGee et al., 1965; Radhakrishnan, 1967) and in more distant galaxies (Roberts, 1967) were unsuccessful. The first detection of an OH transition, in absorption against the radio continuum of NGC 253 and 3034 (Weliachew, 1971), went almost unnoticed because the results were unconvincing. However, Whiteoak and Gardner (1973) and Nguyen-Q-Rieu et al. (1976) confirmed the existence of the absorption.


1973 ◽  
Vol 52 ◽  
pp. 237-241
Author(s):  
J. H. Cahn ◽  
R.D. Nosek

Using the Shklovsky-Minkowski-Aller constant mass method of distances to planetary nebulae, a model of the Galactic dust distribution in the vicinity of the Sun has been determined. Distances are determined in part from extinctions derived from radio continuum to Hβ flux ratios for an assumed electron temperature of 7000 K. The distance scale is based on the brightness of planetary nebulae in the Magellanic Clouds (Seaton, 1968).


1999 ◽  
Vol 190 ◽  
pp. 165-167
Author(s):  
M. Filipović ◽  
L. Staveley-Smith ◽  
R. Haynes ◽  
G. White ◽  
P. Jones

We review all radio-continuum surveys of the Magellanic Clouds (MCs) and also present latest results from our new mosaic surveys.


1991 ◽  
pp. 31-35
Author(s):  
U. Klein ◽  
R. F. Haynes ◽  
R. Wielebinski ◽  
S. R. Wayte ◽  
J. I. Harnett ◽  
...  

Author(s):  
U. Klein ◽  
R. F. Haynes ◽  
D. Meinert ◽  
R. Wielebinski

1998 ◽  
Vol 130 (3) ◽  
pp. 421-440 ◽  
Author(s):  
M. D. Filipović ◽  
R. F. Haynes ◽  
G. L. White ◽  
P. A. Jones

1996 ◽  
Vol 120 (1) ◽  
pp. 77-81 ◽  
Author(s):  
M. D. Filipović ◽  
G. L. White ◽  
R. F. Haynes ◽  
P. A. Jones ◽  
D. Meinert ◽  
...  

1998 ◽  
Vol 130 (3) ◽  
pp. 441-448 ◽  
Author(s):  
M. D. Filipović ◽  
P. A. Jones ◽  
G. L. White ◽  
R. F. Haynes

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