Rise of the intensity of interstellar CH + in the spectrum of AE Aur
Author:
Affiliation:
1. Rzeszów University Rzeszów Poland
2. Instituto de AstronomiaUniversidad Catolica del Norte Antofagasta Chile
3. Pulkovo Observatory Saint‐Petersburg Russia
4. ICAMER ObservatoryNAS of Ukraine Kyiv Ukraine
Funder
Chilean
Polish National Center for Science
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.202013650
Reference20 articles.
1. Observations of Interstellar H and k, Molecular Lines, and Radial Velocities in the Spectra of 300 O and B Stars.
2. CH(+) in the interstellar medium
3. MIKE: A Double Echelle Spectrograph for the Magellan Telescopes at Las Campanas Observatory
4. CO emission and variable CH and CH+absorption towards HD 34078: evidence for a nascent bow shock?
5. Cosentino R. Lovis C. Pepe F. et al.2012 SPIE Conf. Ser. Vol. 8446 1.
Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. ExoMol line lists – LII. Line lists for the methylidyne cation (CH+);Monthly Notices of the Royal Astronomical Society;2023-12-19
2. Spectral investigation of the interstellar cloud towards a runaway star AE Aur;Monthly Notices of the Royal Astronomical Society;2023-09-07
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