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Unveiling the Interplay between the GASP Jellyfish Galaxy JO194 and Its Environment with Chandra

  • Authors: Chiara Bartolini, Alessandro Ignesti, Myriam Gitti, Fabrizio Brighenti, Anna Wolter, Alessia Moretti, Benedetta Vulcani, Bianca M. Poggianti, Marco Gullieuszik, Jacopo Fritz, Neven Tomičić

Chiara Bartolini et al 2022 The Astrophysical Journal 936 .

  • Provider: AAS Journals

Caption: Figure 5.

Ratio between the observed X-ray luminosities, L X,obs, of the total and disk region shown in the Table 4, and the X-ray luminosity associated to the SFR, L X,SFR (Equation (5)). The first four models refer to the Total region of the galaxy and the others to the Disk. The first apec ICM represents the contribution of the ICM emission, except for the last two that represent the contribution of the galaxy’s disk emission. The apec GAL component describes the X-ray emission of a single-temperature plasma, cemekl GAL represents a multitemperature plasma, and mkcflow GAL represents a multiphase gas in radiative cooling. The dashed gray line points L X,obs/L X,SFR = 1.

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