Seminars
 
00/00/0000 - 08/06/2012
Magnetized dense cores: observational characterization and comparison with models
Sala Polivalente C5/1066 (Campus UAB, Bellaterra) (Sala Polivalente C5/1066 (Campus UAB, Bellaterra))
Quiescent and nearby molecular dense cores are ideal targets to study the initial conditions for the formation of relatively isolated low mass stars.
00/00/0000 - 01/06/2012
Unveiling the super-orbital modulation of LS I +61?303 in X-rays
Sala Polivalente C5/1066 (Campus UAB, Bellaterra)
I will briefly introduce my work on gamma-ray binaries and later focus on the super-orbital modulation of LS I +61?303 in X-rays.
00/00/0000 - 25/05/2012
GGD 27: A unique example of high mass star formation
Sala de Grauss II (torre C5 parell 1a planta) (Bellaterra)
GGD 27 is a dense molecular harboring the formation of massive, early B-type stars.
00/00/0000 - 18/05/2012
The Large Scale Universe
Asociació Astronòmica de Sant Cugat - Casa de la Cultura de Sant Cugat (Sant Cugat, Barcelona)
El coneixement de l?Univers com un tot, el seu origen, les lleis que obeeix, la seva forma i les seves dimension, la seva evolució, el seu futur han intrigat desde sempre l?ésser humà.
00/00/0000 - 16/05/2012
The Initial Conditions for Gravitational Collapse of a Low-MassStar-Forming Core
Bellaterra (TBA)
Without accurate knowledge of the initial conditions of gravitational collapsing process of a molecular cloud core, one cannot understand how a low-mass protostar forms.
00/00/0000 - 16/05/2012
Magnetic Field in The Isolated Massive Dense Clump IRAS 20126+4104
Bellaterra (Sala Polivalent 1066)
We measured polarized dust emission at 350 micron towards the high-mass star forming massive dense clump IRAS 20126+4104 using the SHARC II Polarimeter, SHARP, at the Caltech Submillimeter Observatory.
00/00/0000 - 09/05/2012
Magnetic Field in The Isolated Massive Dense Clump IRAS 20126+4104
Bellaterra (TBA)
We measured polarized dust emission at 350 micron towards the high-mass star forming massive dense clump IRAS 20126+4104 using the SHARC II Polarimeter, SHARP, at the Caltech Submillimeter Observatory.
00/00/0000 - 09/05/2012
The Initial Conditions for Gravitational Collapse of a Low-MassStar-Forming Core
Bellaterra (Sala Polivalent 1066)
Without accurate knowledge of the initial conditions of gravitational collapsing process of a molecular cloud core, one cannot understand how a low-mass protostar forms.
00/00/0000 - 07/05/2012
Dark energy modified gravity and Little rip
NTNU, Physics inst. (Trondheim, Norway)
Abstract: review of little Rip cosmology in scalar and modified gravity is given.
00/00/0000 - 04/05/2012
GALACTIC SOURCES MONITORED BY THE FERMI GAMMA-RAY BURST MONITOR
Sala de Graus II (Bellaterra)
More than three years after the launch of the Fermi Gamma-ray Space Telescope, both of its scientific instruments are continuing to make breakthroughs in astrophysics, particle physics, and atmospheric science.
00/00/0000 - 04/05/2012
Why the cosmic roots of life are in the Cosmos?
Llibreria La Rambla, Tarragona (Llibreria Rambla, Rambla Nova nº 99, 43001 Tarragona, Spain)
Stars are the source of all chemical elements, but those generated in the Big Bang. We can keep the memory of Solar System origins from stars by studying primitive meteorites.
00/00/0000 - 00/00/0000
ICCUB PhD lecture. Ignasi Pérez Ràfols: “The cross-correlation among tracers of the underlying large-scale mass distribution in the universe”
The work presented in this Ph.D. thesis is mostly related to the measurement and interpretation of the cross-correlation of different tracers. This is achieved using spectroscopic data from the BOSS survey.
Generalitat de CatalunyaUniversitat de BarcelonaUniversitat Autònoma de BarcelonaUniversitat Politècnica de CatalunyaConsejo Superior de Investigaciones CientíficasCentres de Recerca de Catalunya