Precise Constraints on the Energy Budget of WASP-121 b from Its JWST NIRISS/SOSS Phase Curve

Ultra-hot Jupiters exhibit day-to-night temperature contrasts upwards of 1000 K due to competing effects of strong winds, short radiative timescales, magnetic drag, and H _2 dissociation/recombination. Spectroscopic phase curves provide critical insights into these processes by mapping temperature d...

وصف كامل

التفاصيل البيبلوغرافية

المؤلفون الرئيسيون:	Jared Splinter, Louis-Philippe Coulombe, Robert C. Frazier, Nicolas B. Cowan, Emily Rauscher, Lisa Dang, Michael Radica, Sean Collins, Stefan Pelletier, Romain Allart, Ryan J. MacDonald, David Lafrenière, Loïc Albert, Björn Benneke, René Doyon, Ray Jayawardhana, Doug Johnstone, Vigneshwaran Krishnamurthy, Caroline Piaulet-Ghorayeb, Lisa Kaltenegger, Michael R. Meyer, Jake Taylor, Jake D. Turner
التنسيق:	Artigo
اللغة:	Inglês
منشور في:	IOP Publishing 2025-01-01
سلاسل:	The Astronomical Journal
الموضوعات:	Exoplanets Exoplanet atmospheres Exoplanet atmospheric dynamics Exoplanet systems Exoplanet astronomy Exoplanet atmospheric structure
الوصول للمادة أونلاين:	https://doi.org/10.3847/1538-3881/ae0e52
الوسوم:	إضافة وسم لا توجد وسوم, كن أول من يضع وسما على هذه التسجيلة!