A benchmark for multi-conjugated AO: VLT-MAD observations of the young massive cluster Trumpler 14

Details A benchmark for multi-conjugated AO: VLT-MAD observations of the young massive cluster Trumpler 14 A benchmark for multi-conjugated AO: VLT-MAD observations of the young massive cluster Trumpler 14

2011-08-03

arxiv.org/abs/1108.0905v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

Accepted for publication in MNRAS, 12 pages, 10 figures, 2 tables

Scientific paper

MAD is the first multi-conjugated adaptive optics system at the VLT. We present H and Ks observations of the young massive cluster Trumpler 14 revealing the power of MCAO systems by providing a homogeneous Strehl ratio over a large field of view. Mean Strehl ratios of 6.0 and 5.9 per cent with maximum Strehl ratios of 9.8 and 12.6 per cent in H and Ks, respectively, show significant improvement of the spatial PSF stability compared to single-conjugated adaptive optics systems. Photometry of our observations cover a dynamic range of ~10 mag including 2-3 times more sources than comparable seeing-limited observations. The colour-magnitude diagram reveals that the massive cluster originated in a recent starburst-like event 1+/-0.5 Myr ago. We tentatively detect hints for an older population of 3 Myr suggesting that low intensity star formation might have been going on in the HII region for a few Myr. We derive the luminosity function and mass function between 0.1 M_sun and 3.2 M_sun and identify a change of the power law slope of the mass function at m_c~0.53(+0.12/-0.10) M_sun. The MF appears shallow with power law slopes of Gamma1=-0.50+/-0.11 above m_c and Gamma2=0.63+/-0.32 below m_c.

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