The outer wind of γ Velorum
Author:
Affiliation:
1. Astrophysics, Department of Physics; University of Oxford; DWB, Keble Road; Oxford; OX1 3RH
2. Department of Physics and Astronomy; University College London; Gower Street; London; WC1E 6BT
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/427/1/581/18238618/427-1-581.pdf
Reference28 articles.
1. The infrared spectrum of Velorum
2. Physical Processes in Gaseous Nebulae. III. The Balmer Decrement.
3. The determination of wind terminal velocities and ionic abundances from infrared fine-structure lines: the WC8 component of Velorum
4. On the Excitation of C III in Wolf-Rayet Envelopes
5. The Absolute Magnitudes and Spectral Types of the Stars in the Gamma Velorum System.
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1. Oxygen abundance of γ Vel from [O iii] 88 μm Herschel/PACS spectroscopy;Monthly Notices of the Royal Astronomical Society;2024-01-13
2. Speckle imaging of γ2 Velorum: the inner wind possibly resolved;Monthly Notices of the Royal Astronomical Society;2023-08-17
3. Some important notes on ASTA software: A new method of analysis of simple and complex emission and absorption spectral lines;Astronomy and Computing;2019-01
4. Optical intensity interferometry through atmospheric turbulence;Monthly Notices of the Royal Astronomical Society;2016-02-05
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