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B. Davies

3 papers hereh-index 6179 citations13 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author1
  • last author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
  • astro-ph.HE1
same name
  • B. Davies — 40 papers, h 32
  • B. Davies — 24 papers, h 16
  • B. Davies — 23 papers, h 18
  • B. Davies — 6 papers, h 3
  • B. Davies — 3 papers, h 7
  • B. Davies — 2 papers, h 18

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20232026
collaborators

3 papers

astro-ph.HE2026

JWST spectroscopy of SN 2010da/NGC 300 ULX-1: a surviving star hidden by dust

Emma R. Beasor, Ryan Lau, Nathan Smith +3

We present new James Webb Space Telescope (JWST) NIRSpec and MIRI integral-field spectroscopy of the remarkable system SN~2010da / NGC~300 ULX-1, the only known ultraluminous X-r…

astro-ph.SR2025

Variable Polarization of WR~31a: Binary Companion or Co-Rotating Interaction Region?

Christiana Erba, Richard Ignace, Faith Simmons +1

WR 31a (Hen 3-519) is likely a post-luminous blue variable (LBV) star that is evolving to become a classical Wolf-Rayet star. Multicolor (UBVR) photopolarimetric observations of WR…

astro-ph.SR2023

The effect of winds on atmospheric layers of red supergiants II. Modelling VLTI/GRAVITY and MATISSE observations of AH Sco, KW Sgr, V602 Car, CK Car and V460 Car

G. González-Torà, M. Wittkowski, B. Davies +1

Mass loss plays a crucial role in the lives of massive stars, especially as the star leaves the main sequence and evolves to the red supergiant (RSG) phase. However, the physical p…

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