adsabs/AstroCLIMB huggingface dataset:
Paper: A Two-zone Accretion Disk in the Changing-look Active Galactic Nucleus 1ES 1927+654: Physical Implications for Tidal Disruption Events and Super-Eddington Accretion
Authors: Ruancun Li, Luis C. Ho, Claudio Ricci, Benny Trakhtenbrot
Figure caption: The Eddington ratio (λ E) as a function of the dimensionless mass accretion rate (﹩\dot{m}﹩), color-coded by the time since the outburst (2017 December 23), from the beginning (green) to the end (red), where the orange one denotes t ≈ 650 days. The red star shows the value in 2011 May, before the outburst. The dotted line marks the ﹩{\lambda }_{{\rm{E}}}-\dot{m}﹩ relation with constant radiation efficiency η = 0.08, while the dashed line denotes η = 0.03. The blue solid line shows the ﹩{\lambda }_{{\rm{E}}}-\dot{m}﹩ relation for a typical slim accretion disk (M. A. Abramowicz et al. 1988). The open gray squares represent the six extreme narrow-line Seyfert 1 galaxies in C. Jin et al. (2023), and the open diamonds are derived from the super-Eddington accretion flows in the two-dimensional radiation-hydrodynamic simulations of K. Ohsuga et al. (2005).
Paper: Can Supernovae from Runaway Stars Mimic the Signs of Absorbing “Supervirial” Gas?
Authors: Mukesh Singh Bisht, Projjwal Banerjee, Biman B. Nath, Yuri Shchekinov
Figure caption: Evolution of oxygen column density of the shocked ejecta with time for density profiles with different core sizes of β = 0, 0.15, 0.3, and 0.5 shown in red, green, magenta, and blue, respectively. For no core case (β = 0), we use a constant oxygen mass fraction of 0.15 throughout the ejecta. The dotted vertical lines in the respective color show the time when the reverse shock hits the center of the ejecta. The curves correspond to the adopted fiducial values of E = 1051 erg, M ej = 10 M ⊙, and n 0 = 0.1 cm−3.