Yesterday May 23rd, a group of Members of the European Parliament belonging to the Regional Development Commission visited the Installations of the Roque de los Muchachos Observatory (ORM). They also were given informatjon about the use of the European Funds for Regional Development which have been used to build world class sceintiric installations such as the Gran Telescopio Canarias, and the telescopes of the CTA (Cherenkov Telescope Array). The visit was in the framework of the visit by the Commisson to the island of La Palma to see directly the consequences of the eruption of the volcano
This section includes scientific and technological news from the IAC and its Observatories, as well as press releases on scientific and technological results, astronomical events, educational projects, outreach activities and institutional events.
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Spanish Minister of Science and Innovation, Diana Morant, visited last Wednesday the Centre for Astrophysics’ facilities in La Palma (CALP) to know the impact of the volcanic eruption on the personnel and on the operation of the facilities at the Roque de los Muchachos Observatory (Garafía, La Palma). During her visit, she held a meeting with IAC Director Rafael Rebolo, which was also attended by the Director of the Gran Telescopio Canarias (GTC), Romano Corradi, and the ORM Site Manager, Juan Carlos Pérez Arencibia. Accompanying the Minister were the General Secretary of Research, Raquel
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One of the most interesting questions for astrophysicists for the past few decades is how and when did the first galaxies form. One of the possible answers to “how” is that star formation in the first galaxies took place at a steady rate, building up a system with increasing mass. Another possibility is that the formation was more violent and discontinuous, with intense bursts of star formation, on short timescales, triggered by events such as galaxy mergers and strong concentrations of gas.
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Newly formed stars have protoplanetary discs around them. A fraction of the material in the disc condenses into planet-forming chunks, and the rest finally falls into the star. Because of their common origin, researchers have assumed that the composition of these chunks and that of the rocky planets with low masses should be similar to that of their host stars. However, until now the Solar System was the only available reference for the astronomers.
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All the main components of the new multiobject spectrograph WEAVE on the William Herschel Telescope (WHT) in the Roque de los Muchachos Observatory (Garafía, La Palma) have arrived on the island. The Instituto de Astrofísica de Canarias (IAC) has played an outstanding role in the design and production of the parts of this instrument, the work of an international collaboration, which will start its commissioning after immediate integration on the telescope.
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An international team of scientists led from the Centre for Astrobiology (CAB, CSIC-INTA), with participation from the Instituto de Astrofísica de Canarias (IAC), has used the Gran Telescopio Canarias (GTC) to study a representative sample of galaxies, both disc and spheroidal, in a deep sky zone in the constellation of the Great Bear to characterize the properties of the stellar populations of galactic bulges. The researchers have been able to determine the mode of formation and development of these galactic structures. The results of this study were recently published in The Astrophysical
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