Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
Scientist
INAF-OA Italia
Torino Obs
Torino Observ., Italy
INAF, Osservatorio Astronomico di Torino, Italy
OATo, Torino, Italy
OATo Torino;
INAF-Oss. Astronomico di Torino
INAF, Astronomical Obs. Torino, I-10025 Torino, Italy
INAF_OA Torino, Italy
INAF Torino Astronomical Obs.;
INAF, Torino Astronomical Observatory, Pino Torinese, Torino, Italy
INAF-OATo, Pino Torinese, Italy
Osservatorio Astronomico di Torino, Strada Osservatorio 20, 10025 Pino Torinese, Italy
Osservatorio Astronomico di Torino, Pino Torinese, Italy
Turin Astronomical Observatory, National Institute of Astrophysics
Scuola Internazionale Superiore di Studi Avanzati, Trieste, Italy
Osservatorio Astronomico di Torino, I-10025 Pino Torinese, Italy
Osservatorio Astronomico di Torino, Strada Osservatorio 20, I-10025 Pino Torinese, Italy
INAF, Osservatorio Astronomico di Torino, I-10025 Pino Torinese, Torino, Italy
INAF, Osservatorio Astronomico di Torino, Via Osservatorio 20, 10025 Pino Torinese, Italy
CNR, Istituto di Cosmogeofisica; Torino, Università, Turin, Italy
TO
Osservatorio Astronomico di Torino, I-10025, Pino Torinese, Italy
Torino, Osservatorio Astronomico, Pino Torinese, Italy
Osservatorio Astronomico Torino, St. da Osservatorio 20, 10025 Pino Torinese, Italy
Turin Univ., Italy.
INAF-OATo, Via Osservatorio 20, 10025 Pino Torinese, Italy
Osservatorio Astronomico di Torino, Strada Osservatorio 20, Pino Torinese, I-10025, Italy.
Osservatorio Astronomico di Torino, Torinese, Italy
Osservatorio Astronomico di Torino, Torino, Italy
The Astronomer Organization, Birmingham, UK
Istituto di Fisica Generale dell'Università, Torino, Italy
Inst. di Fisica Generale dell'Univ., Torino, Italy
Osservatorio Astronomico di Torino
A beaming model for the OJ 287 periodic optical outbursts
A helical jet model to explain the Mkn 501 SED variations
A multiwavelength study of the OJ 287 variability
A neutron process during Ne shell burning in massive stars.
A new activity phase of the blazar 3C 454.3. Multifrequency observations by the WEBT and XMM-Newton in 2007-2008
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