Sergio Molinari
0000-0002-9826-7525
Istituto di Astrofisica e Planetologia Spaziali
334 papers found
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The LWS calibration strategy
ISO long wavelength spectrometer interactive analysis system
The Formation of Massive Stars. I. High‐Resolution Millimeter and Radio Studies of High‐Mass Protostellar Candidates
Far-Infrared Spectroscopy of the HH 1/2 Outflow
High-Mass Protostars
FIRST and the Formation of Massive Stars
Star Formation in Clusters: from ISO to FIRST
Infrared and Millimetric Study of the Young Outflow Cepheus E
An Infrared Study of the L1551 Star Formation Region - What We Have Learnt from ISO and the Promise for FIRST
Search for CO Outflows toward a Sample of 69 High-Mass Protostellar Candidates: Frequency of Occurrence
Multi-wavelength analysis of IRAS 23011+6126 and its young embedded outflow.
A molecular-line study of clumps with embedded high-mass protostar candidates
A Shock‐induced Photodissociation Region in the HH 80/81 Flow: Far‐Infrared Spectroscopy
The LWS Interactive Analysis (LIA) Package
An infrared study of the L1551 star formation region
Molecular Outflows from High Mass Protostars
The ISO-LWS map of the Serpens cloud core. I. The SEDs of the IR/SMM sources
Infrared Space ObservatorySpectroscopy of HH 7–11 Flow and Its Redshifted Counterpart
Far infrared spectroscopy of FU Ori objects. ISO-LWS observations
The structure of the collapsing envelope around the low-mass protostar IRAS 16293-2422
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