High angular resolution near-infrared integral field observations of young star cluster complexes in NGC 1365

E. Galliano; M. Kissler-Patig; D. Alloin; E. Telles

doi:10.1051/0004-6361/201218812

Free Access

Issue		A&A Volume 545, September 2012


Article Number		A10
Number of page(s)		15
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/201218812
Published online		28 August 2012

Online material

	Fig. 9 Set of plots showing different relations between observables. The plots are described in Sect. 4.2. In all plots, the cyan dots correspond to the sources M4, M5, M5-2 to M5-4 and M6. The red dots correspond to the apertures chosen in the H₂ image.
Open with DEXTER

Table 1

Results from the measurements described in Sect. 3.2 for the apertures defined in the K-band image.

Table 2

Measurements described in Sect. 3.2, for the apertures defined on the Brγ image and the H₂ image.

Table 3

Measurements described in Sect. 3.2, for the apertures defined on the Brγ image and the H₂ image.

Table 4

Measurements described in Sect. 3.2, for the apertures defined on the Brγ image and the H₂ image.

© ESO, 2012

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