The Signature of a Windy Radio Supernova Progenitor in a Binary System. The curious case of SN1979C in which ripples observed in radio can be explained by the interaction of the wind of the supernova progenitor with a companion star in relatively wide orbit.
收藏DataCite Commons2022-02-02 更新2024-07-28 收录
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https://figshare.com/articles/dataset/The_Signature_of_a_Windy_Radio_Supernova_Progenitor_in_a_Binary_System_The_curious_case_of_SN1979C_in_which_ripples_observed_in_radio_can_be_explained_by_the_interaction_of_the_wind_of_the_supernova_progenitor_with_a_companion_star_in_relat/7243178/1
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资源简介：
Simulation of the wind of a 18MSun (ZAMS) star shortly before it explodes in a supernova, in orbit around a 15MSun companion star. The simulation is for the last 14000 years before the supernova explosion. simulations are performed using AMUSE, with Fi as the hydro code and Huayno for integrating the planetary orbit.Mass per SPH particle is 10e-5MSun, orbital period is 2000yrs, circular. Binary plan is in the X-Y plane.<br>datafiles containing particle data from the simulations.snapshot_000xxx_gas.amuse (35 in total)snapshot_000xxx_stars.amuse (35 in total)<br>datafiles containinig observations of SN1979C:SN1979C_488GHz_fit.csv (fitted data) <br>SN1979C_488GHz.csv (raw data)<br>plotting routines:compare_lightcurve.pyplot_pd.py
提供机构：
figshare
创建时间：
2020-08-28
