Discovery of a Red Supergiant Donor Star in SN2010da/NGC 300 ULX-1-Reference-Cited by-同舟云学术

Discovery of a Red Supergiant Donor Star in SN2010da/NGC 300 ULX-1

Published:2019-09-25 Issue:2 Volume:883 Page:L34
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Heida M.^ORCID,Lau R. M.,Davies B.^ORCID,Brightman M.,Fürst F.^ORCID,Grefenstette B. W.^ORCID,Kennea J. A.^ORCID,Tramper F.^ORCID,Walton D. J.^ORCID,Harrison F. A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/ab4139/pdf

Reference64 articles.

1. Modelling optical emission of Ultra-luminous X-ray Sources accreting above the Eddington limit

2. Astropy: A community Python package for astronomy

3. An ultraluminous X-ray source powered by an accreting neutron star

4. The first gravitational-wave source from the isolated evolution of two stars in the 40–100 solar mass range

5. No Strong Geometric Beaming in the Ultraluminous Neutron Star Binary NGC 300 ULX-1 (SN 2010da) from Swift and Gemini

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