Physical Properties of the Host Galaxies of Ca-rich Transients

Calcium-rich (Ca-rich) transients are a new class of supernovae (SNe) that are known for their comparatively rapid evolution, modest peak luminosities, and strong nebular calcium emission lines. Currently, the progenitor systems of Ca-rich transients remain unknown. Although they exhibit spectroscop...

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Veröffentlicht in:	arXiv.org 2022-02
Hauptverfasser:	Dong, Y, Milisavljevic, D, Leja, J, Sarbadhicary, S K, Nugent, A E, Margutti, R, Jacobson-Galan, W V, Polin, A, Banovetz, J, Reynolds, J M, Subrayan, B
Format:	Artikel
Sprache:	eng
Schlagworte:	Calcium Explosions Galaxies Massive stars Metallicity Physical properties Star & galaxy formation Star formation rate Stellar evolution Stellar mass Stellar populations Supernovae Transients (astronomy) White dwarf stars White dwarfs
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