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X-WR-CALNAME:Instituto de Astrofísica de Andalucía
X-ORIGINAL-URL:https://www.iaa.csic.es
X-WR-CALDESC:Eventos para Instituto de Astrofísica de Andalucía
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TZID:Europe/Paris
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DTSTART:20250330T010000
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DTSTART:20251026T010000
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DTSTART:20260329T010000
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DTSTART:20261025T010000
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DTSTART:20270328T010000
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DTSTART:20271031T010000
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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260514T123000
DTEND;TZID=Europe/Paris:20260514T133000
DTSTAMP:20260407T054631
CREATED:20260119T144357Z
LAST-MODIFIED:20260312T154846Z
UID:29183-1778761800-1778765400@www.iaa.csic.es
SUMMARY:TBD
DESCRIPTION:TBD \nFecha y lugar: 14/05/2026 – 12:30 | Salón de ActosGwenaël Alan MilcareckIAA-CSIC \n  \n  \n  \n 
URL:https://www.iaa.csic.es/evento/tbd-2/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260521T123000
DTEND;TZID=Europe/Paris:20260521T133000
DTSTAMP:20260407T054631
CREATED:20260302T161002Z
LAST-MODIFIED:20260302T161005Z
UID:30049-1779366600-1779370200@www.iaa.csic.es
SUMMARY:SO Colloquium - Models for Protostellar Molecular Jets
DESCRIPTION:TBD \nFecha y lugar: 21/05/2026 – 12:30 | Salón de ActosSylvie CabritObservatory of Paris\, France \n  \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-models-for-protostellar-molecular-jets/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260526T123000
DTEND;TZID=Europe/Paris:20260526T133000
DTSTAMP:20260407T054631
CREATED:20260302T161423Z
LAST-MODIFIED:20260302T161427Z
UID:30054-1779798600-1779802200@www.iaa.csic.es
SUMMARY:TBD
DESCRIPTION:TBD \nFecha y lugar: 26/05/2026 – 12:30 | Salón de ActosMario TafallaObservatorio Astronómico Nacional \n  \n  \n  \n 
URL:https://www.iaa.csic.es/evento/tbd-4/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260528T123000
DTEND;TZID=Europe/Paris:20260528T133000
DTSTAMP:20260407T054631
CREATED:20260302T161538Z
LAST-MODIFIED:20260326T105423Z
UID:30058-1779971400-1779975000@www.iaa.csic.es
SUMMARY:What the Variability of Embedded Protostars Tells Us about Accretion: Past\, Present\, and Future
DESCRIPTION:The James Clerk Maxwell Telescope (JCMT) has been monitoring eight nearby low-mass star-forming regions in the Gould Belt at submillimetre wavelengths for more than eight years to search for and quantify the time dependent brightness variability of the resident deeply embedded protostars. \nSecular variability is common among these protostars; greater than 25% of the sample show measurable long-term brightness changes and 10% show burst behaviour lasting months to years. We interpret this secular variability as reflecting changes in the mass accretion rate from the disk to the protostar\, as predicted by theoretical models of (proto)stellar assembly. For a subset of our sample we have contemporaneous mid-IR light-curves which allow additional constraints on the conditions responsible for the brightness variations\, confirming that the submillimetre variability is driven by changes in the dust temperature profile of the envelope. \nFurthermore\, we have combined\, for one source\, single dish and interferometric sub-mm monitoring\, which has allowed us to unambiguously recover a time lag in the variability at larger angular scales and use the results to confirm the envelope structure surrounding the embedded protostar. \nFecha y lugar: 28/05/2026 – 12:30 | Salón de ActosDoug JohnstoneNational Research Council Canada – Herzberg Astronomy and Astrophysics Research Centre \n  \n 
URL:https://www.iaa.csic.es/evento/what-the-variability-of-embedded-protostars-tells-us-about-accretion-past-present-and-future/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260618T123000
DTEND;TZID=Europe/Paris:20260618T133000
DTSTAMP:20260407T054631
CREATED:20260123T100555Z
LAST-MODIFIED:20260123T100559Z
UID:29319-1781785800-1781789400@www.iaa.csic.es
SUMMARY:TBD
DESCRIPTION:TBD \nFecha y lugar: 18/06/2026 – 12:30 | Salón de ActosSilvia CelliSapienza University of Rome \n  \n  \n  \n 
URL:https://www.iaa.csic.es/evento/tbd-3/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20261022T123000
DTEND;TZID=Europe/Paris:20261022T133000
DTSTAMP:20260407T054631
CREATED:20260323T094624Z
LAST-MODIFIED:20260323T095004Z
UID:30339-1792672200-1792675800@www.iaa.csic.es
SUMMARY:Venus as an Anchor Point for Planetary Habitability
DESCRIPTION:A fundamental aspect of understanding the limits of habitable environments and detectable signatures is the study of where the boundaries of such environments can occur\, and the conditions under which a planet is rendered into a hostile environment. In our solar system\, Venus is the most Earth-like planet\, yet at some point in planetary history there was a bifurcation between the two: Earth has been continually habitable since the end-Hadean\, whereas Venus became uninhabitable. Indeed\, Venus is the type-planet for a world that has transitioned from habitable and Earth-like conditions\, through the inner edge of the Habitable Zone (HZ); thus it provides a natural laboratory to study the evolution of habitability. \nIn this talk I will describe the gaps in our knowledge regarding Venus within the context of how these gaps are impacting our ability to model exoplanet atmospheres and interiors. I will discuss various factors that relate to a possible habitable past of Venus\, including orbital evolution. I will outline exoplanet target selection for testing the conditions of runaway greenhouse and present examples of potential Venus analogs. \nFinally\, I will summarize the primary exoplanet science questions that will be addressed by the coming NASA and ESA missions to Venus. \n  \nFecha y lugar: 22/10/2026 – 12:30 | Salón de ActosStephen KaneUniversity of California\, Riverside \n 
URL:https://www.iaa.csic.es/evento/venus-as-an-anchor-point-for-planetary-habitability/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
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