scholarly journals Hierarchical Structures of Medium-Scale Cyclones and Cloud Clusters near the Baiu Front Observed by MU and Meteorological Radars: Outline and Preliminary Results of Three-Week Observation Campaign.

1996 ◽  
Vol 48 (1) ◽  
pp. 151-160 ◽  
Author(s):  
Y. Shibagaki ◽  
M. D. Yamanaka ◽  
H. Uyeda ◽  
A. Watanabe ◽  
Y. Maekawa ◽  
...  
Keyword(s):  
Hierarchical Structures ◽  
Medium Scale ◽  
Preliminary Results ◽  
Cloud Clusters ◽  
Baiu Front

Preliminary Results of the Medium Scale Anisotropy Measurement1

1993 ◽  
Vol 688 (1) ◽  
pp. 801-803
Author(s):  
J. Puchalla ◽  
E. Cheng ◽  
D. Cottingham ◽  
D. Fixsen ◽  
E.P. Gentieu ◽  
...  
Keyword(s):  
Medium Scale ◽  
Preliminary Results

scholarly journals A Survey of Magellanic Cloud Clusters for RR Lyrae Stars

1984 ◽  
Vol 108 ◽  
pp. 37-38
Author(s):  
J. A. Graham ◽  
J. M. Nemec
Keyword(s):  
Variable Stars ◽  
Magellanic Cloud ◽  
Magellanic Clouds ◽  
The Other ◽  
Rr Lyrae Stars ◽  
Preliminary Results ◽  
Rr Lyrae ◽  
Other Hand ◽  
Cloud Clusters ◽  
Lyrae Stars

Preliminary results are presented of a search for RR Lyrae variable stars in old clusters in the Magellanic Clouds. RR Lyraes have been found in NGC 1786 and NGC 2210. With the exceptions of NGC 339 (SMC) and NGC 2019 and Hodge 11 (LMC), all clusters classified as type VII by Searle, Wilkinson and Bagnuolo (1980) contain RR Lyrae variables. On the other hand, none have yet been found in clusters of type VI.

scholarly journals Young Magellanic Cloud Clusters (< 1 Gyr): Census, Properties, Star Formation History

1999 ◽  
Vol 190 ◽  
pp. 405-409 ◽  
Author(s):  
Eva K. Grebel ◽  
Dennis Zaritsky ◽  
Jason Harris ◽  
Ian Thompson
Keyword(s):  
Star Formation ◽  
Age Distribution ◽  
Magellanic Clouds ◽  
Star Formation History ◽  
Stellar Content ◽  
Preliminary Results ◽  
Cloud Clusters ◽  
Formation History ◽  
Cluster Properties ◽  
Cluster Age

We report preliminary results from an automated cluster survey of the Magellanic Clouds aimed at improving the cluster census and at deriving cluster properties from their resolved stellar content. The survey is tripling the number of known clusters. The cluster age distribution shows similar peaks at 100–200 Myr in LMC and SMC, coincident with the closest encounter of the Clouds and perigalacticon.

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