activity
20042009
most citedPast and present star formation in the SMC: NGC 346 and its neighborhood

111 citations · 474 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2009★ 59 cited

Star formation history in the SMC: the case of NGC602

M. Cignoni, E. Sabbi, A. Nota +9

Deep HST/ACS photometry of the young cluster NGC 602, located in the remote low density "wing" of the Small Magellanic Cloud, reveals numerous pre-main sequence stars as well as yo…

astro-ph2008★ 51 cited

A New Hubble Space Telescope Distance to NGC 1569: Starburst Properties and IC 342 Group Membership

Aaron J. Grocholski, Alessandra Aloisi, Roeland P. van der Marel +8

We present deep HST ACS/WFC photometry of the dwarf irregular galaxy NGC 1569, one of the closest and strongest nearby starburst galaxies. These data allow us, for the first time,…

astro-ph2007★ 77 cited

The Stellar Mass Distribution in the Giant Star Forming Region NGC 346

E. Sabbi, M. Sirianni, A. Nota +8

Deep F555W and F814W Hubble Space Telescope ACS images are the basis for a study of the present day mass function (PDMF) of NGC346, the largest active star forming region in the Sm…

astro-ph2007★ 64 cited

Starbursts in the Local Universe: new HST/ACS observations of the irregular galaxy NGC 4449

F. Annibali, A. Aloisi, J. Mack +5

We present photometry with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope (HST) of stars in the Magellanic starburst galaxy NGC 4449. The galaxy has been image…

astro-ph2006★ 111 cited

Past and present star formation in the SMC: NGC 346 and its neighborhood

E. Sabbi, M. Sirianni, A. Nota +8

In the quest of understanding how star formation occurs and propagates in the low metallicity environment of the Small Magellanic Cloud (SMC), we acquired deep F555W (~V), and F814…

astro-ph2005★ 36 cited

Dynamical and chemical evolution of NGC1569

S. Recchi, G. Hensler, L. Angeretti +1

Blue Compact Dwarf and Dwarf Irregular galaxies are generally believed to be unevolved objects, due to their blue colors, compact appearance and large gas fractions. Many of these…