9 citations · 9 across the 2 of their papers we have counts for
3 papers
astro-ph.SR2026
Astrophysical parameters of LS 437 and the nature of X0726-260
Ignacio Negueruela, Sara R. Berlanas, Lee J. Townsend +2
Be/X-ray binaries, the most common class of high-mass X-ray binaries, are characterised by OBe companions, but display a rich variety of X-ray behaviours. One of the most atypical…
astro-ph.SR2023★ 9 cited
To clump or not to clump The impact of wind inhomogeneities on the optical and NIR spectroscopic analysis of massive OB stars
K. Rübke, A. Herrero, J. Puls
Winds of massive stars have density inhomogeneities (clumping) that may affect the formation of spectral lines in different ways, depending on their formation region. Most of previ…
astro-ph.IM2022
Web-based telluric correction made in Spain: spectral fitting of Vega-type telluric standards
D. de la Fuente, A. Marco, L. R. Patrick +7
Infrared spectroscopic observations from the ground must be corrected from telluric contamination to make them ready for scientific analyses. However, telluric correction is often…