AAVSO How to [Python! Visualizing MESA models with TULIPS]
AAVSo webinar
Instructor: Eva Laplace (Heidelberg Institute for Theoretical Studies--HITS)
Please note: Dr. Laplace has provided links for you to download and install Tulips prior to her presentation: https://www.aavso.org/sites/default/files/education/presentations/How-toTulip_Instructions_12.22.pdf
In this third How to Python! broadcast, Dr. Eva Laplace will teach attendees how to use her Python package, TULIPS, to visualize MESA models. MESA models track the changing temperature, radius, composition, and structure of stars as they evolve, making them valuable tools for stellar researchers; but they are famously difficult to use. TULIPS makes it easy to visualize complex information, allowing you to create beautiful plots and animations showing the changes a star will undergo during its lifetime. Knowledge of basic Python is recommended. Attendees are encouraged to familiarize themselves with TULIPS ahead of time: https://pypi.org/project/astro-tulips/
Our previous How to Python webinars will help you become familiar with Python:
The basics: https://www.youtube.com/watch?v=7eMTgQuKGHA&list=PLnZ_rvnR35rfGTaq4g3kzVOfkna1JeDyX&index=7&t=2s
Finding Frequency Solutions for Variable Star Light Curves: https://www.youtube.com/watch?v=ZhtHBkbTuWY&t=3s
Join us for our 2023 webinars!
www.aavso.org/programs-events
Видео AAVSO How to [Python! Visualizing MESA models with TULIPS] канала AAVSO HQ
Instructor: Eva Laplace (Heidelberg Institute for Theoretical Studies--HITS)
Please note: Dr. Laplace has provided links for you to download and install Tulips prior to her presentation: https://www.aavso.org/sites/default/files/education/presentations/How-toTulip_Instructions_12.22.pdf
In this third How to Python! broadcast, Dr. Eva Laplace will teach attendees how to use her Python package, TULIPS, to visualize MESA models. MESA models track the changing temperature, radius, composition, and structure of stars as they evolve, making them valuable tools for stellar researchers; but they are famously difficult to use. TULIPS makes it easy to visualize complex information, allowing you to create beautiful plots and animations showing the changes a star will undergo during its lifetime. Knowledge of basic Python is recommended. Attendees are encouraged to familiarize themselves with TULIPS ahead of time: https://pypi.org/project/astro-tulips/
Our previous How to Python webinars will help you become familiar with Python:
The basics: https://www.youtube.com/watch?v=7eMTgQuKGHA&list=PLnZ_rvnR35rfGTaq4g3kzVOfkna1JeDyX&index=7&t=2s
Finding Frequency Solutions for Variable Star Light Curves: https://www.youtube.com/watch?v=ZhtHBkbTuWY&t=3s
Join us for our 2023 webinars!
www.aavso.org/programs-events
Видео AAVSO How to [Python! Visualizing MESA models with TULIPS] канала AAVSO HQ
Показать
Комментарии отсутствуют
Информация о видео
Другие видео канала
AAVSO webinar with its Bright Star Monitor Observing SectionAAVSO webinar with Dr. Emily Levesque and Dariusz KubickiAAVSO How [My Students and I do Science With AAVSO Data--and How You Can, Too]AAVSO Webinar, with its Short Period Pulsator Observing SectionMeet the AAVSO's Exoplanet, YSO, and I&E SectionsLas Estrellas a tu Alcance: Erupciones, "apagones" y variabilidad: la vida de T TauriLa Ciencia del Cielo para Principiantes: Ciencia CiudadanaMembership MeetingEclipsing Binaries Observing Section Webinar109th Annual Meeting, Solar Observing session (2020)AAVSO Spectroscopy Workshop, Day2 (2020)Meet the AAVSO's CV, SPP, and AAVSOnet SectionsLa Ciencia del Cielo para Principiantes: ISS y ArtemisSolar Observing Section WebinarAAVSO How-to Hour: A Quick Guide to VSX, with Sebastián OteroAAVSO Webinar, with Dr. Luisa Rebull and Dr. Margarita KarovskaHow to model isochrones using images of star clustersLong Period Variables Observing Section webinarJune 6, 2022 Open House recordingAmateur Astronomy with the AAVSO (with captioning)AAVSO webinar, with Francois Cochard: New to Spectroscopy? A few tips to start successfully