no code implementations • 25 Feb 2021 • J. A. Toalá, P. Jiménez-Hernández, J. B. Rodríguez-González, S. Estrada-Dorado, M. A. Guerrero, V. M. A. Gómez-González, G. Ramos-Larios, D. A. García-Hernández, H. Todt
Gas and dust masses for the born-again ejecta in A30 are estimated to be $M_\mathrm{gas}=(4. 41^{+0. 55}_{-0. 14})\times10^{-3}$ M$_\odot$ and $M_\mathrm{dust}=(3. 20^{+3. 21}_{-2. 06})\times10^{-3}$ M$_\odot$, which can be used to estimate a total ejected mass and mass-loss rate for the born-again event of $(7. 61^{+3. 76}_{-2. 20})\times10^{-3}$ M$_{\odot}$ and $\dot{M}=[5-60]\times10^{-5}$ M$_{\odot}$ yr$^{-1}$, respectively.
Astrophysics of Galaxies Solar and Stellar Astrophysics
