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Items: 7

1.

Complex Organic Molecules tracing shocks along the outflow cavity in the high-mass protostar IRAS 20126+4104.

Palau A, Walsh C, Sánchez-Monge Á, Girart JM, Cesaroni R, Jiménez-Serra I, Fuente A, Zapata LA, Neri R.

Mon Not R Astron Soc. 2017 Jun;467(3):2723-2752.

2.

The critical role of disks in the formation of high-mass stars.

Cesaroni R, Galli D, Lodato G, Walmsley M, Zhang Q.

Nature. 2006 Dec 7;444(7120):703-6.

PMID:
17151657
3.

Infall of gas as the formation mechanism of stars up to 20 times more massive than the Sun.

Beltrán MT, Cesaroni R, Codella C, Testi L, Furuya RS, Olmi L.

Nature. 2006 Sep 28;443(7110):427-9.

PMID:
17006508
4.

Shock-heated NH3 in a Molecular Jet Associated with a High-Mass Young Star.

Zhang Q, Hunter TR, Sridharan TK, Cesaroni R.

Astrophys J. 1999 Dec 20;527(2):L117-L120.

PMID:
10577953
5.

The independence of face identity and facial expression recognition mechanisms: relationship to sex and cognitive style.

Pizzamiglio L, Zoccolotti P, Mammucari A, Cesaroni R.

Brain Cogn. 1983 Apr;2(2):176-88.

PMID:
6546021
7.

[Correlated endoscopic-radiologic study for diagnostic assessment of lesions in the duodenal bulb].

Cesaroni R, Mieli C, Nava G.

Minerva Gastroenterol. 1974 Apr-Jun;20(2):55. Italian. No abstract available.

PMID:
4423721

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