The massive binary system 9 Sgr revisited: New insights into disentangling methods-Reference-Cited by-同舟云学术

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The massive binary system 9 Sgr revisited: New insights into disentangling methods

Published:2020-07 Issue:6-7 Volume:341 Page:628-637
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron. Nachr

Author:

Quintero Edwin A.¹²,Eenens Philippe¹,Rauw Gregor³

Affiliation:

1. Departamento de Astronomía Universidad de Guanajuato Guanajuato Mexico

2. Observatorio Astronómico (OAUTP) Universidad Tecnológica de Pereira Risaralda Colombia

3. Space Sciences, Technologies and Astrophysics Research (STAR) Institute Université de Liège Liège Belgium

Funder

Universidad de Guanajuato

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.202013696

Reference23 articles.

1. Tomographic separation of composite spectra - The components of the O-star spectroscopic binary AO Cassiopeiae

2. Fundamental stellar and accretion disc parameters of the eclipsing binary DQ Velorum

3. The new Wolf-Rayet binary system WR62a

4. Spectroscopic Studies of O-Type Stars. I. Classification and Absolute Magnitudes

5. The Quadruple Wolf‐Rayet System GP Cephei: Spectral Types, Masses, Mass‐Loss Rate, and Colliding Winds

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1. Using a new spectral disentangling approach to ascertain whether the massive binary HDE 228766 contains a Wolf–Rayet star;Monthly Notices of the Royal Astronomical Society;2024-07-05

2. The B-type Binaries Characterisation Programme – II. VFTS 291: a stripped star from a recent mass transfer phase;Monthly Notices of the Royal Astronomical Society;2023-09-01

3. New insight into the massive eccentric binary HD 165052: self-consistent orbital solution, apsidal motion, and fundamental parameters;Monthly Notices of the Royal Astronomical Society;2023-03-14

4. Fundamental parameters for double-lined spectroscopic and detached eclipsing binary system J064726.39 + 223431.6;Monthly Notices of the Royal Astronomical Society;2022-12-22

5. Ultraviolet Spectropolarimetry: on the origin of rapidly rotating B stars;Astrophysics and Space Science;2022-12

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