| Issue |
EAS Publications Series
Volume 71-72, 2015
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
|
|
|---|---|---|
| Page(s) | 147 - 148 | |
| Section | Binaries | |
| DOI | https://doi.org/10.1051/eas/1571031 | |
| Published online | 01 December 2015 | |
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 147-148
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 147-148
Molecular Formation in Classical Novae: The Case of V2676 Oph
1 Koyama Astronomial Observatory, Kyoto Sangyo University, Motoyama, Kamigamo, Kita-ku, Kyoto 603–8555, Japan
2 Fujii-Kurosaki Observatory, 4500 Kurosaki, Tamashima, Kurashiki, Okayama 713–8126, Japan
Molecular formation of C2 and CN in a dust-forming classical nova V2676 Oph occurred at temperatures <6000 K. Such conditions were probably achived by the UV absorption of C I, Fe II, and etc..
© EAS, EDP Sciences, 2015