Variable O Vi And N V Emission From The X-ray Binary Lmc X-3: Heating Of The Black Hole Companion*

2025/04/19 by Song, L, Tripp, TM, Wang, QD +8
#Astrophysics and Astronomy #stars: individual (LMCX-3)

paper · doi:10.7275/2154

Abstract

This is the pre-published version harvested from ArXiv. The published version is located at http://iopscience.iop.org/1538-3881/140/3/794

Related

• Black Hole X-ray Binaries Lmc X–1 And X–3: Observations Confront Spectral Models
• Warm-hot Gas In And Around The Milky Way: Detection And Implications Of Ovii Absorption Toward Lmc X-3
• Ultraluminous X-ray Source 1e 0953.8+6918 (m81 X-9): An Intermediate-mass Black Hole Candidate And Its Environs
• Probing O Vi Emission In The Halos Of Edge-on Spiral Galaxies
• X-ray And Ultraviolet Spectroscopy Of Galactic Diffuse Hot Gas Along The Large Magellanic Cloud X-3 Sight Line