Surveys for Planetary Nebulae in the Magellanic Clouds

2006 ◽  
pp. 17-29 ◽  
Author(s):  
George H. Jacoby
Keyword(s):  
Planetary Nebulae ◽  
Magellanic Clouds

Planetary Nebulae in the Magellanic Clouds

2001 ◽  
pp. 203-204
Author(s):  
P. Leisy ◽  
M. Dennefeld
Keyword(s):  
Planetary Nebulae ◽  
Magellanic Clouds

Physical Properties of the Central Stars of Planetary Nebulae in the Magellanic Clouds

1983 ◽  
pp. 373-373
Author(s):  
T. P. Stecher ◽  
S. P. Maran ◽  
T. R. Gull ◽  
L. H. Aller ◽  
M. P. Savedoff
Keyword(s):  
Physical Properties ◽  
Planetary Nebulae ◽  
Magellanic Clouds ◽  
Central Stars

Stellar Evolution in the Magellanic Clouds from Studies of Planetary Nebulae

1992 ◽  
pp. 502-502
Author(s):  
N. A. Walton ◽  
M. J. Barlow ◽  
D. J. Monk ◽  
R. E. S. Clegg
Keyword(s):  
Stellar Evolution ◽  
Planetary Nebulae ◽  
Magellanic Clouds

Spectrophotometry of Selected Planetary Nebulae of Type I in the Magellanic Clouds

1993 ◽  
pp. 584-584
Author(s):  
S. Torres-Peimbert ◽  
M. Peimbert ◽  
M. T. Ruitz ◽  
M. Peña
Keyword(s):  
Planetary Nebulae ◽  
Magellanic Clouds ◽  
Type I

The Magellanic Clouds and Planetary Nebulae

1984 ◽  
pp. 363-374 ◽  
Author(s):  
Manuel Peimbert
Keyword(s):  
Planetary Nebulae ◽  
Magellanic Clouds

scholarly journals Large-scale structure of the Magellanic Clouds using planetary nebulae

1991 ◽  
Vol 148 ◽  
pp. 89-95
Author(s):  
S. J. Meatheringham
Keyword(s):  
Large Scale ◽  
Planetary Nebulae ◽  
Large Scale Structure ◽  
Magellanic Clouds ◽  
Scale Structure ◽  
The Galaxy ◽  
Young Clusters

The Small and Large Magellanic Clouds (SMC, LMC) are of considerable interest from a kinematical viewpoint. The tidal interation of the Clouds with each other and with the Galaxy appears to have been quite significant in recent times (Murai & Fujimoto 1980). The SMC in particular appears to have been considerably disrupted by a recent close passage to the LMC (Mathewson & Ford 1984, Mathewson 1984, Mathewson et al. 1986). For the LMC Freeman et al. (1983) found that the young and old populations have significantly different rotation solutions.Planetary Nebulae (PN) form a population with age intermediate between the HI and young clusters and the old Population II clusters. A large number of PN are known in the MCs. Sanduleak et al. (1978) compiled a list of 102 in the LMC and 28 in the SMC. Since then other authors have increased the total number known to approximately 140 in the LMC and 50 in the SMC.

scholarly journals Planetary Nebulae in the Magellanic Clouds

1999 ◽  
Vol 190 ◽  
pp. 332-338 ◽  
Author(s):  
Michael A. Dopita
Keyword(s):  
Hubble Space Telescope ◽  
Morphological Structure ◽  
Planetary Nebulae ◽  
Spectroscopic Studies ◽  
Magellanic Clouds ◽  
Star Formation History ◽  
Formation History ◽  
History Of ◽  
Central Stars ◽  
The Ideal

The proximity, accurately known distance and low line-of-sight reddening give the ideal circumstances to pursue studies of individual stellar populations in the Magellanic Clouds. Here we show how our understanding of the evolution and chemical composition of the planetary nebulae in the Magellanic Clouds has been impacted by imaging and UV spectroscopic studies using the Hubble Space Telescope. Images provide sizes, internal morphological structure, absolute fluxes, and dynamical ages, while spectra allow us to place the central stars accurately on the H-R Diagram, and we can also examine the details of the evolution, of mass- and age- dependent chemical dredge-up processes, and infer the star-formation history of the Magellanic Clouds.

scholarly journals Spectroscopic Observations of Planetary Nebulae in the Magellanic Clouds

1968 ◽  
Vol 34 ◽  
pp. 34-35 ◽  
Author(s):  
M. W. Feast
Keyword(s):  
Planetary Nebulae ◽  
Magellanic Clouds ◽  
Preliminary Results ◽  
Spectroscopic Observations

A programme of spectroscopic observations of planetary nebulae in both Magellanic Clouds has been underway in Pretoria for some years, and some preliminary results for the LMC have been published (Feast, 1964b). More extensive observations are now available (altogether in both clouds 112 spectra of 39 objects), and these are being prepared for publication elsewhere. Below are summarized the main conclusions so far deduced.

scholarly journals Radio planetary nebulae in the Magellanic Clouds

2011 ◽  
Vol 7 (S283) ◽  
pp. 334-335 ◽  
Author(s):  
Evan J. Crawford ◽  
Miroslav D. Filipović ◽  
Ivan S. Bojičić ◽  
Martin Cohen ◽  
Jeff L. Payne ◽  
...  
Keyword(s):  
Planetary Nebulae ◽  
Magellanic Clouds ◽  
Radio Continuum ◽  
Preliminary Results ◽  
Compact Array

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

Planetary nebulae as standard candles. VI - A test in the Magellanic Clouds

1990 ◽  
Vol 365 ◽  
pp. 471 ◽  
Author(s):  
George H. Jacoby ◽  
Robin Ciardullo ◽  
Alistair R. Walker
Keyword(s):  
Planetary Nebulae ◽  
Magellanic Clouds
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