Supernova remnants destroy interstellar dust less efficiently per event in dense high-star-formation regions than in the Milky Way's diffuse medium, with destruction maximized when thermal sputtering time matches the remnant age and scaling linearly with metallicity.
Similarity and Dimensional Methods in Mechanics
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2verdicts
UNVERDICTED 2representative citing papers
42 supernova remnants confirmed in NGC3344 via [S II]/Hα selection, Sabbadin plots, BPT diagrams and shock models from SITELLE data.
citing papers explorer
-
Destruction of the interstellar dust by a supernova
Supernova remnants destroy interstellar dust less efficiently per event in dense high-star-formation regions than in the Milky Way's diffuse medium, with destruction maximized when thermal sputtering time matches the remnant age and scaling linearly with metallicity.
-
3D Optical Spectroscopic Study of NGC3344 with SITELLE: I. Identification and Confirmation of Supernova Remnants
42 supernova remnants confirmed in NGC3344 via [S II]/Hα selection, Sabbadin plots, BPT diagrams and shock models from SITELLE data.