Figure 5 from A Highly Eccentric Warm Jupiter Orbiting TIC 237913194

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A Highly Eccentric Warm Jupiter Orbiting TIC 237913194

Authors: Martin Schlecker, Diana Kossakowski, Rafael Brahm, Néstor Espinoza, Thomas Henning, Ludmila Carone, Karan Molaverdikhani, Trifon Trifonov, Paul Mollière, Melissa J. Hobson, Andrés Jordán, Felipe I. Rojas, Hubert Klahr, Paula Sarkis, Gáspár Á. Bakos, Waqas Bhatti, David Osip, Vincent Suc, George Ricker, Roland Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Michael Vezie, Jesus Noel Villaseñor, Mark E. Rose, David R. Rodriguez, Joseph E. Rodriguez, Samuel N. Quinn, and Avi Shporer

2020 The Astronomical Journal 160 275.

Provider: AAS Journals

Caption: Figure 5.

Evolution of the planetary equilibrium temperature in the case of instantaneous heat adjustment for different albedos α and re-radiation factors β. We assumed unity infrared emissivity ﹩{\varepsilon }_{\mathrm{IR}}﹩. Black lines denote the time of transit and secondary eclipse, respectively. Due to the high eccentricity, ﹩{T}_{\mathrm{eq},\mathrm{inst}}﹩ varies by several hundred Kelvin within one orbit. It stays below 1000 K for most of the orbit.

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