Planetary nebulae (PN) are one of the final phases in the evolution of
low and intermediate mass stars (<8 Msun). They display a great variety
of shapes, although in their previous phases (Asymptotic giant branch
Thursday, November 28, 2013 - 13:30
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In this talk -my last one in the IAA for the moment- I will talk
The European VLBI Network (EVN) is currently the most sensitive VLBI array in the world (its collecting area is about a hundred thousand square meters, or 1/10 of the planned Square Kilometer Array).
Thursday, October 31, 2013 - 13:30
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The science performed in Astronomy is digital science, from observing proposals to final publication, including data and software used: each of the elements and actions involved in the scientific output could be recorded in electronic form.
SN1993J, a powerful radio supernova high in the northern sky, has been monitored with VLBI though its lifetime. The VLBI observations have been phase-referenced to the core of M81.
Thursday, July 18, 2013 - 14:30
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The International Conference on Phenomena in Ionized Gases (ICPIG) is bringing together over five hundred researchers in Granada this week
ICPIG - 2013: International Conference on Phenomena in Ionized Gases
2013-07-14 00:00:00 to 2013-07-19 00:00:00
Granada
ICPIG - 2013: International Conference on Phenomena in Ionized Gases
The ALHAMBRA (Advance Large Homogeneous Area Medium Band Redshift
Astronomical; Moles et al. 2008) survey has observed 8 different regions
of the sky, including sections of the COSMOS, DEEP2, ELAIS, GOODS-N, SDSS
Thursday, June 27, 2013 - 14:30
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tbd
Thursday, June 20, 2013 - 14:30
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Thursday, June 13, 2013 - 14:30
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Note:
This is a seminar given at the European Research Council Headquarter some weeks ago.
It was focused on the expected audience, members of the ERC directly involved in
setting the rules for Grants evaluation and/or participate in all steps of the
Jets 2013: The Innermost Regions of Relativistic Jets and Their Magnetic Fields
2013-06-10 00:00:00 to 2013-06-14 00:00:00
Granada
Jets 2013: The Innermost Regions of Relativistic Jets and Their Magnetic Fields