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3.23. The centre of the LMC bar

Published online by Cambridge University Press:  25 May 2016

A. Ardeberg ,
P. Linde ,
R. Snel ,
B. Gustafsson  and
P. E. Nissen
A. Ardeberg
Affiliation:
Lund Observatory Box 43, 221 00 Lund, Sweden
P. Linde
Affiliation:
Lund Observatory Box 43, 221 00 Lund, Sweden
R. Snel
Affiliation:
Lund Observatory Box 43, 221 00 Lund, Sweden
B. Gustafsson
Affiliation:
Astron. Obs., Uppsala Univ. Box 515, 751 20 Uppsala, Sweden
P. E. Nissen
Affiliation:
Inst. Phys. Astron., Aarhus Univer. Aarhus, Denmark

Extract

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We study star formation and chemical evolution in the LMC Bar centre with the HST PC and uvby photometry. For all bands, mean turn off star data have σ around 0.015 mag. Present data have zero points from stars in M67. b-y of these stars coincides with target turn off. All measurement bands have zero point accuracy better than 0.010 mag.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 135 - 136
Copyright
Copyright © Kluwer 1998