The contribution of Oxygen to the "30", "26" and "20" μm features

Astronomy and Astrophysics

Volumn 362, Issue 2, 2000, Pages

  Papoular, R ^a  

^a CEA SACLAY   (France)

Author keywords

Infrared: ISM: lines and bands; ISM: dust, extinction; ISM: Planetary nebulae: general; Molecular processes; Radiation mechanisms: thermal

Indexed keywords

EID: 0002587812     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (3)

1. Behar F. and Vandenbroucke M. 1986, Rev. Inst. Fr. Petrole,41,2
2. Cody J. Jr at al. 1990, in Cody G, Geballe T. and Sheng P., Physical phenomena in granular materials, MRS Symp. Proc. 195, MRS, Pittsburgh
3. Forrest W., Houck J. and McCarthy J. 1981, ApJ 248, 195