ISOCAM Observations of Globular Clusters in the Magellanic Clouds: The Data

Details ISOCAM Observations of Globular Clusters in the Magellanic Clouds: The Data ISOCAM Observations of Globular Clusters in the Magellanic Clouds: The Data

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004apjs..155..401t&link_type=abstract

The Astrophysical Journal Supplement Series, Volume 155, Issue 2, pp. 401-419.

Astronomy and Astrophysics

Astronomy

5

Galaxies: Star Clusters, Infrared: Stars, Galaxies: Magellanic Clouds, Stars: Agb And Post-Agb, Stars: Evolution

Scientific paper

Seventeen globular clusters in the Large and Small Magellanic Clouds were observed in the mid-infrared wavelength region with the ISOCAM instrument on board the Infrared Space Observatory (ISO). Observations were made using the broadband filters LW1, LW2, and LW10, corresponding to the effective wavelengths of 4.5, 6.7, and 12 μm, respectively. We present the photometry of point sources in each cluster, as well as their precise positions and finding charts.
Based on observations with ISO, an ESA project with instruments funded by ESA Member states (especially the PI countries: France, Germany, the Netherlands and the United Kingdom) and with participation of ISAS and NASA.

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