... Home Page of FRANCESCO FONTANI . Research Interests: high-massstar formation. ... to the formation and evolution of massivestars is a fundamental tool to investigate ...
... away, shows a bright, rapidly rotating massivestar surrounded by a disk of gas ... the small companion was actually the most massivestar in the system and because of ...
... 2005, A , in press . Triggered Massive-Star Formation on the Borders of Galactic HII Regions II. ... Riccardo Cesaroni . 2005, Proceedings of the IAUS227 "MassiveStar Birth: A Crossroads of Astrophysics", in press . ...
... Photoevaporation of Disks and Clumps By Nearby MassiveStars: . ... of the Trapezium showing the four energetic massivestars and a plethora of Sun-like ... head and a tail pointing directly away from the energetic central massivestars ...
... 1999, A , in press . Low massstars in the massive HII region NGC 3603 . ... Series, in press . Young massivestars in the ISOGAL survey. ... molecular cores and the earliest phases of high-massstar formation ( Table 1 , Fig ...
... ratios as a tracer of accelerated collapse in regions of high massstar formation ... 2004, ApSS, in press . Star clusters near intermediate and high massstars . ... Current views on low-massstar formation . Francesco Palla . ...
... Massivestar-formation toward G28.87+0.07 (IRAS 18411-0338) investigated by means of ... Influence of Magnetic Fields in Low-MassStar Formation . Pau FRAU . ... Probing the earliest phases of high-massstar formation through observations of N2D ...
... 2002, ApJ, in press . Probes of high massstar formation . M. Walmsley . ... Near and Mid-infrared images of the massivestar forming complex G9.62+0.19 , ( PDF ... 2002, A 388, L9 . Young massivestars in the ISOGAL survey. II. ...
... The critical role of disks in the formation of high-massstars . ... Triggered massive-star formation on the borders of Galactic HII regions. III. ... interfaces between outflows and ambient cloud in high-massstar forming regions ...
... Leiden Obser vator y) 0.5 Fraction contributed by recycling 0.4 35% 19% SFR Stellar mass AGB stars SN Type Ia Massivestars 0.3 Cosmological SPH simulation: Evolution and Assembly of GaLaxies and their Environments (EAGLE) At z = 0, 35% of the cosmic SFR ...