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Properties of LMC Planetary Nebulae and parent populations in the MACHO database

Published online by Cambridge University Press:  25 May 2016

D.R. Alves
Affiliation:
1UC Davis/LLNL
C. Alcock
Affiliation:
2LLNL
R. A. Allsman
Affiliation:
3ANUSF
T. S. Axelrod
Affiliation:
4MSSSO/LLNL
A. C. Becker
Affiliation:
6CfPA/U Wash.
D. R. Bennett
Affiliation:
7Notre Dame
K. H. Cook
Affiliation:
2LLNL
K. C. Freeman
Affiliation:
5MSSSO
K. Griest
Affiliation:
8CfPA/UCSD
J. Guern
Affiliation:
8CfPA/UCSD
M. J. Lehner
Affiliation:
8CfPA/UCSD
S. L. Marshall
Affiliation:
2LLNL
D. Minniti
Affiliation:
2LLNL
B. A. Peterson
Affiliation:
5MSSSO
P. J. Quinn
Affiliation:
9ESO
M. R. Pratt
Affiliation:
6CfPA/U Wash.
A. W. Rodgers
Affiliation:
5MSSSO
C. W. Stubbs
Affiliation:
6CfPA/U Wash.
W. Sutherland
Affiliation:
10Oxford
D. Welch
Affiliation:
11McMaster

Abstract

The MACHO microlensing experiment's time-sampled photometry database contains blue and red lightcurves for nearly 9 million stars in the central bar region of the Large Magellanic Cloud (LMC). We have identified known LMC Planetary Nebulae (PN) in the database and find one, Jacoby 5, to be variable. We additionally present data on the “parent populations” of LMC PN, and discuss the star formation history of the LMC bar.

Type
VIII. Planetary Nebulae in Extragalactic Systems
Copyright
Copyright © Kluwer 1997 

References

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