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X-WR-CALNAME:Instituto de Astrofísica de Andalucía
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X-WR-CALDESC:Eventos para Instituto de Astrofísica de Andalucía
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DTSTAMP:20260419T040531
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SUMMARY:Academic Spanish Course for Foreigners (2025)
DESCRIPTION:The Academic Spanish course for foreigners is designed to facilitate effective communication in academic and profesional contexts. Through a practical and personalized focus\, the participants will develop essential linguistic abilities to discuss scientific articles\, participate in conferences\, give presentations\, and collaborate in international projects. The program includes technical vocabulary\, beginner and advanced grammar\, and simulations of real-life situations. Moreover\, it will promote the cultural immersion to strengthen the comprehension of the Hispanic world\, and their impact on interdisciplinary investigation and collaboration. \nThis course will be taught throughout in the following blocks: \nJanuary 21st – February 27thApril 22nd – May 29thSeptember 23rd – October 30thThe course is taught by Prof. Nazira Ruíz
URL:https://www.iaa.csic.es/evento/academic-spanish-course-for-foreigners-2025/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
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DTSTART;TZID=Europe/Paris:20250408T123000
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CREATED:20250407T074050Z
LAST-MODIFIED:20250407T074109Z
UID:25302-1744115400-1744119000@www.iaa.csic.es
SUMMARY:Synthetic ngVLA Observations of Ionized Gas in Massive Protostars and Future Prospects for Protoplanetary Disk Studies with ngVLA and SKA
DESCRIPTION:The study of protoplanetary disks is essential for understanding stellar evolution and the origins of planets. However\, these systems present significant observational challenges due to their small angular size\, low surface brightness\, and complex structure. Radio interferometry provides a unique advantage by observing dust and gas at wavelengths that penetrate the dense regions where the protoplanetary disk forms. The upcoming Next Generation Very Large Array (ngVLA) will transform protoplanetary disk studies with its unprecedented angular resolution and sensitivity in the millimeter and centimeter bands. These capabilities will allow high-fidelity imaging of disk substructures\, planet-disk interactions\, and dust evolution\, offering critical insights into the processes shaping planetary systems. The Square Kilometre Array (SKA) will complement these efforts by detecting cold molecular gas\, magnetic fields\, and ionized material\, providing additional constraints on disk dynamics and chemistry. Together\, these facilities will enable a multi-scale\, multi-phase perspective on planet-forming environments. \nA major challenge associated with these observatories is the immense volume of data they will generate and the necessitating advanced deconvolution and imaging techniques to reconstruct high-fidelity images. In this talk\, I will present results from simulated ngVLA observations of ultracompact HII regions (Jáquez-Domínguez et al. 2025) and my current work on protoplanetary disks\, where I am testing the capabilities and optimal configurations of ngVLA and SKA to maximize their scientific performance. By combining state-of-the-art radiative transfer models with next-generation imaging techniques\, we aim to refine strategies for future high-resolution disk studies. These efforts will be crucial for unlocking the full potential of ngVLA and its synergy with SKA and ALMA\, paving the way for transformative discoveries in planet formation. \nFecha: 08/04/2025 – 12:30Conferenciante: Dr. Miguel JáquezFiliación: IRyA (UNAM)\, México \n 
URL:https://www.iaa.csic.es/evento/synthetic-ngvla-observations-of-ionized-gas-in-massive-protostars-and-future-prospects-for-protoplanetary-disk-studies-with-ngvla-and-ska/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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