Rise of the intensity of interstellar CH+ in the spectrum of AE Aur
- 1 January 2020
- journal article
- research article
- Published by Wiley in Astronomische Nachrichten
- Vol. 341 (1), 56-63
- https://doi.org/10.1002/asna.202013650
Abstract
No abstract availableKeywords
Funding Information
- Chilean (CONICYT REDES 180136)
- Polish National Center for Science (UMO-2017/25/B/ST9/01524)
This publication has 14 references indexed in Scilit:
- State-to-state chemistry and rotational excitation of CH+ in photon-dominated regionsMonthly Notices of the Royal Astronomical Society, 2017
- Interstellar HydridesAnnual Review of Astronomy and Astrophysics, 2016
- Dense molecular globulettes and the dust arc toward the runaway O star AE Aurigae (HD 34078)Astronomy & Astrophysics, 2014
- Variable interstellar lines in spectra of HD 73882Publications of the Astronomical Society of the Pacific, 2013
- CO emission and variable CH and CH+absorption towards HD 34078: evidence for a nascent bow shock?Astronomy & Astrophysics, 2009
- The BOES Spectropolarimeter for Zeeman Measurements of Stellar Magnetic FieldsPublications of the Astronomical Society of the Pacific, 2007
- MIKE: A Double Echelle Spectrograph for the Magellan Telescopes at Las Campanas ObservatoryPublished by SPIE-Intl Soc Optical Eng ,2003
- Examination of the Interstellar Spectrum of AE Aur for Long‐Term ChangesPublications of the Astronomical Society of the Pacific, 1999
- CH(+) in the interstellar mediumThe Astrophysical Journal, 1994
- Observations of Interstellar H and k, Molecular Lines, and Radial Velocities in the Spectra of 300 O and B Stars.The Astrophysical Journal, 1949