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The absolute-magnitude distributions of seven supernova types are presented. The data used here were primarily taken from the Asiago Supernova Catalogue, but were supplemented with additional data. We accounted for both foreground and host-galaxy ext
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5492d1201919ba4aef042d76688e1ac4
Publikováno v:
AIP Conference Proceedings.
Hard X‐ray emission associated with white dwarfs (WDs) can be used to diagnose the presence of late‐type binary companions, mass accretion from companions, or physical processes with unknown origins. Since our previous systematic searches for har
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::12d84bb9a9d233d372560df677d8e2c7
https://doi.org/10.1063/1.3527783
https://doi.org/10.1063/1.3527783
