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The Orion Nebula in the mid-IR
M. Robberto, S. V. W. Beckwith, N. Panagia +6
We present two wide-field (5'x5'), diffraction limited, broad-band 10 and 20 micron images of the Orion Nebula, plus six 7-13 micron narrow-band images of BN/KL taken at the 3.8m U…
Massive Star Feedback on the IMF
M. Robberto, J. Song, G. Mora Carrillo +3
We have obtained the first measures of the mass accretion rates on stars of the Trapezium Cluster. They appear systematically lower than those of similar stars in the Taurus-Auriga…
The Initial Conditions to Star Formation: Low Mass Stars at Low Metallicity
Martino Romaniello, Nino Panagia, Massimo Robberto
We have measured the present accretion rate of roughly 800 low-mass (~1-1.4 Mo) pre-Main Sequence stars in the field of SN 1987A in the Large Magellanic Cloud. The stars with stati…
Low-Mass Pre-Main Sequence Stars in the Large Magellanic Cloud - III: Accretion Rates from HST-WFPC2 Observations
Martino Romaniello, Massimo Robberto, Nino Panagia
We have measured the present accretion rate of roughly 800 low-mass (~1-1.4 Mo) pre-Main Sequence stars in the field of Supernova 1987A in the Large Magellanic Cloud (LMC, Z~0.3 Zo…
HST/WFPC2 Study of the Trapezium Cluster: the Influence of Circumstellar Disks on the Initial Mass Function
M. Robberto, J. Song, G. Mora Carrillo +3
We have performed the first measures of mass accretion rates in the core of the Orion Nebula Cluster. Four adjacent fields centered on the Trapezium stars have been imaged in the U…