Spitzer Infrared Spectrograph (IRS) Observations of Large Magellanic Cloud Planetary Nebula SMP 83

2004 ◽  
Vol 154 (1) ◽  
pp. 271-274 ◽  
Author(s):  
J. Bernard‐Salas ◽  
J. R. Houck ◽  
P. W. Morris ◽  
G. C. Sloan ◽  
S. R. Pottasch ◽  
...  
Keyword(s):  
Planetary Nebula ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud

scholarly journals A More Complete Listing of LMC Planetary Nebulae

1984 ◽  
Vol 108 ◽  
pp. 231-232
Author(s):  
N. Sanduleak
Keyword(s):  
Planetary Nebula ◽  
Planetary Nebulae ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Plate Material ◽  
Schmidt Telescope ◽  
Complete Listing ◽  
Objective Prism

In an earlier paper by Sanduleak et al. (1978) a listing was given of 102 confirmed and probable planetary nebulae in the Large Magellanic Cloud detected on objective-prism plates taken with the Curtis Schmidt telescope at Cerro Tololo. Subsequently, deeper coverage was obtained on nitrogen-baked Kodak IIIa-J plates plus GG 455 filter exposed for 90 minutes. The thin prism was again used to provide a dispersion of about 1500 Å mm−1 at Hβ and the spectra were unwidened. An additional 25 planetary nebula candidates were found on this new plate material to show the requisite characteristics, i.e. they display (a) a stellar appearance, (b) [OIII] λλ5007, 4959 strongly in emission, and (c) no evidence of a continuum.

Spectrophotometric Data of the Central Star of the Large Magellanic Cloud Planetary Nebula N66: Quantitative Analysis of Its WN‐Type Spectrum

1997 ◽  
Vol 491 (1) ◽  
pp. 233-241 ◽  
Author(s):  
M. Pena ◽  
W.‐R. Hamann ◽  
L. Koesterke ◽  
J. Maza ◽  
R. H. Mendez ◽  
...  
Keyword(s):  
Quantitative Analysis ◽  
Planetary Nebula ◽  
Central Star ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Spectrophotometric Data ◽  
Type Spectrum

Large Magellanic Cloud Planetary Nebula Morphology: Probing Stellar Populations and Evolution

2000 ◽  
Vol 534 (2) ◽  
pp. L167-L171 ◽  
Author(s):  
Letizia Stanghellini ◽  
Richard A. Shaw ◽  
Bruce Balick ◽  
J. Chris Blades
Keyword(s):  
Planetary Nebula ◽  
Stellar Populations ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud

scholarly journals SMC 1 or What's in a Name?

1999 ◽  
Vol 190 ◽  
pp. 17-18
Author(s):  
Hélène R. Dickel
Keyword(s):  
Planetary Nebula ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Web Documents

What's in a name? Everything! SMC 1 is a planetary nebula in the Large Magellanic Cloud! URLs of Web documents are given to aid astronomers in designating their astronomical sources so as to avoid confusion in the literature.

Mass Loss Processes in Hot Evolved Stars: Planetary Nebula Nuclei in the Large Magellanic Cloud

1997 ◽  
pp. 470-470
Author(s):  
L. Bianchi ◽  
E. Vassiliadis ◽  
M. A. Dopita
Keyword(s):  
Mass Loss ◽  
Planetary Nebula ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Evolved Stars

scholarly journals The central star of the planetary nebula N 66 in the Large Magellanic Cloud: A detailed analysis of its dramatic evolution 1983–2000

2003 ◽  
Vol 409 (3) ◽  
pp. 969-982 ◽  
Author(s):  
W.-R. Hamann ◽  
M. Peña ◽  
G. Gräfener ◽  
M. T. Ruiz
Keyword(s):  
Detailed Analysis ◽  
Planetary Nebula ◽  
Central Star ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud

scholarly journals The Unusual Variability of the Large Magellanic Cloud Planetary Nebula RPJ 053059-683542

2007 ◽  
Vol 669 (1) ◽  
pp. L25-L28 ◽  
Author(s):  
Richard A. Shaw ◽  
Armin Rest ◽  
Guillermo Damke ◽  
R. Chris Smith ◽  
Warren A. Reid ◽  
...  
Keyword(s):  
Planetary Nebula ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud

Hot Evolved Objects in Different Parent Galaxies: The Stellar Winds of Three Planetary Nebula Nuclei in the Large Magellanic Cloud

1997 ◽  
Vol 480 (1) ◽  
pp. 290-296 ◽  
Author(s):  
Luciana Bianchi ◽  
Emanuel Vassiliadis ◽  
Michael Dopita
Keyword(s):  
Planetary Nebula ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Stellar Winds

scholarly journals Mass loss processes in hot evolved stars: Planetary Nebula nuclei in the large Magellanic Cloud

1997 ◽  
Vol 180 ◽  
pp. 470-470
Author(s):  
L. Bianchi ◽  
E. Vassiliadis ◽  
M. A. Dopita
Keyword(s):  
Mass Loss ◽  
Planetary Nebula ◽  
Strong Dependence ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Stellar Winds ◽  
Element Abundances ◽  
Model Predictions ◽  
Nearby Galaxies ◽  
Ngc 6822

As part of a broad study of stellar winds in different galaxies, to establish observational constraints on the influence of metallicity on the mass loss process, we investigate the winds of planetary nebula (PN) nuclei in the Large Magellanic Cloud. Theoretically, the radiation pressure mechanism implies a strong dependence of the wind acceleration on the element abundances. Observationally, model predictions have been tested using Pop. I stars in the Magellanic Clouds (Puls et al. 1996, A&A, 305, 171) and massive stars in the nearby galaxies M31, M33 and NGC 6822 (Bianchi et al. 1996, AJ, 111, 2303; Bianchi et al. 1996, in prep.). We now extend this investigation to low luminosity, evolved objects.

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