Multiwavelength Study of the X-Ray Bright Supernova Remnant N300-S26 in NGC 300
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab189d/pdf
Reference49 articles.
1. DUST PROCESSING IN SUPERNOVA REMNANTS:SPITZERMIPS SPECTRAL ENERGY DISTRIBUTION AND INFRARED SPECTROGRAPH OBSERVATIONS
2. THE STELLAR ANCESTRY OF SUPERNOVAE IN THE MAGELLANIC CLOUDS. I. THE MOST RECENT SUPERNOVAE IN THE LARGE MAGELLANIC CLOUD
3. Identification of Supernova Remnants in the Sculptor Group Galaxies NGC 300 and NGC 7793
4. THE MAGELLAN/IMACS CATALOG OF OPTICAL SUPERNOVA REMNANT CANDIDATES IN M83
5. Statistical Analysis of Supernova Remnants in the Large Magellanic Cloud
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1. A Panchromatic Study of the X-Ray Binary Population in NGC 300 on Subgalactic Scales;The Astrophysical Journal;2024-07-01
2. A soft and transient ultraluminous X-ray source with six-hour modulation in the NGC\,300 galaxy;Astronomy & Astrophysics;2023-12-14
3. MUSE crowded field 3D spectroscopy in NGC 300;Astronomy & Astrophysics;2022-12
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