A new catalogue of emission-line stars and planetary nebulae in the Small Magellanic Cloud

1961 ◽  
Vol 66 ◽  
pp. 169 ◽  
Author(s):  
E. M. Lindsay
2003 ◽  
Vol 596 (2) ◽  
pp. 997-1014 ◽  
Author(s):  
Letizia Stanghellini ◽  
Richard A. Shaw ◽  
Bruce Balick ◽  
Max Mutchler ◽  
J. Chris Blades ◽  
...  

1999 ◽  
Vol 190 ◽  
pp. 97-98
Author(s):  
P. Frank Winkler ◽  
Yasser Rathore ◽  
R. Chris Smith

We present results on the SMC from the first full season of the Michigan/CTIO Magellanic Cloud Emission-Line Survey, being carried out from CTIO. Images are being obtained in Hα, [S II] λλ 6717, 6731, and [O III] λ 5007, plus red and green continuum bands for star subtraction. Data from the 1996–97 season have been assembled into large mosaic images which reveal the rich variety of nebulosity in the SMC in unprecedented detail. These are providing definitive samples of the active, occasionally violent, ISM on scales including superbubbles, wind-blown bubbles, supernova remnants, H II regions, and planetary nebulae.


2016 ◽  
Vol 361 (3) ◽  
Author(s):  
Howard Leverenz ◽  
Miroslav D. Filipović ◽  
I. S. Bojičić ◽  
E. J. Crawford ◽  
J. D. Collier ◽  
...  

2016 ◽  
Vol 728 ◽  
pp. 072008
Author(s):  
D. Drašković ◽  
Q. A. Parker ◽  
W. A. Reid ◽  
M. Stupar

1984 ◽  
Vol 88 ◽  
pp. 265-268
Author(s):  
E. Maurice ◽  
N. Martin ◽  
L. Prévot ◽  
E. Rebeirot

Kinematical studies of the Magellanic Clouds began more than half a century ago, when Wilson, in 1918, first interpreted the gradient of the 17 radial velocities of gazeous nebulae in the Large Cloud in terms of rotation. In the case of the Small Magellanic Cloud, the first real attempt to understand the velocity field of this galaxy was performed by the Radcliffe astronomers (Feast et al., 1960, 1961). Their study was based on radial velocities of 40 stars and 13 HII regions.With the installation by ESO of an objective-prisme astrograph in South Africa, in 1961, and then of several larger telescopes in Chile in 1968, the number of measurements significantly increased for Magellanic objects, in particular in the SMC. In this galaxy, the objective-prism observations resulted in about 100 stellar radial velocities (Florsch, 1972a) of probable members. A compilation by Maurice (1979) of all then known slit-spectrograph radial velocities gave velocities for 80 supergiants, 35 HII regions and 12 planetary nebulae.


2015 ◽  
Vol 452 (2) ◽  
pp. 1402-1411 ◽  
Author(s):  
Danica Drašković ◽  
Quentin A. Parker ◽  
Warren A. Reid ◽  
Milorad Stupar

1991 ◽  
Vol 148 ◽  
pp. 196-197 ◽  
Author(s):  
M. Meyssonnier ◽  
M. Azzopardi

New identifications of the Hα-emission-line objects in the Small Magellanic Cloud (SMC) have been made with the Curtis Schmidt telescope at Cerro Tololo Inter-American Observatory (CTIO).


1995 ◽  
Vol 148 ◽  
pp. 415-418
Author(s):  
D. H. Morgan

AbstractThis paper describes the results of searches for planetary nebulae on seven objective prism plates which were taken with the UK 1.2m Schmidt Telescope and cover the entire Small Magellanic Cloud. A total of 62 objects were detected; their spatial distribution is discussed.


2007 ◽  
Vol 472 (1) ◽  
pp. 101-110 ◽  
Author(s):  
T. P. Idiart ◽  
W. J. Maciel ◽  
R. D. D. Costa

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