We present Gemini-North GMOS/IFU observations of a young star cluster and its environment near the centre of the dwarf irregular starburst galaxy NGC 1569. This forms part of a larger and ongoing study of the formation and collimation mechanisms of galactic winds, including three additional IFU pointings in NGC 1569 covering the base of the
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Gemini GMOS/IFU spectroscopy of NGC 1569 - I. Mapping the properties of a young star cluster and its environmentWestmoquette, M. S. et al.112007
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Gemini GMOS/integral field unit spectroscopy of NGC 1569 - II. Mapping the roots of the galactic outflow
We present a set of four Gemini-North Multi-Object Spectrograph/integral field unit (IFU) observations of the central disturbed regions of the dwarf irregular starburst galaxy NGC 1569, surrounding the well-known superstar clusters A and B. This continues on directly from a companion paper, in which we describe the data reduction and analysis
Westmoquette, M. S. et al.Fecha de publicación:
112007 -
Geneva photometry of HD 129929 (Aerts+, 2004)
We have gathered and analysed a timeseries of 1493 high-quality multicolour Geneva photometric data of the B3V {beta} Cep star Hd 129929. The dataset has a time base of 21.2 years. The occurrence of a beating phenomenon is evident from the data. We find evidence for the presence of at least six frequencies, among which we see components of two
Aerts, C. et al.Fecha de publicación:
112003 -
Geneva photometry time series of HD 203664 (Aerts+, 2006)
Time series of seven colour Geneva photometry in the filters U B1 B B2 V1 V G of the star HD 203664 (1 data file).
Aerts, C. et al.Fecha de publicación:
112005 -
Global morphology and physical relations between the stars, gas and dust in the disc and arms of M100.
We study star formation processes in the disc of the weakly barred grand design spiral galaxy M100 (NGC 4321) from a variety of images tracing recent massive star formation, old and young stars, dust and neutral hydrogen. Differences between arm and interarm regions are specifically studied by decomposing the images into arm and non-arm zones. We
Knapen, J. H. et al.Fecha de publicación:
111996 -
Globular clusters systems and their host dark matter halos
Not Available
Spitler, L.Fecha de publicación:
112008