Infrared spectrum of eta Carinae: 3--14 microns
Journal Article
·
· Publ. Astron. Soc. Pac., v. 87, no. 520, pp. 917-921
Intermediate resolution spectral scans of eta Car in the range 3.2--14 $mu$m provide strong support for the model proposed by Robinson, Hyland, and Thomas (1973) in which the infrared emission arises from two concentric dust shells heated by the central object. No fine-structure or recombination emission lines were observed over this spectral range. (auth)
- Research Organization:
- State Univ. of New York, Stony Brook
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-33-026987
- OSTI ID:
- 4003974
- Journal Information:
- Publ. Astron. Soc. Pac., v. 87, no. 520, pp. 917-921, Journal Name: Publ. Astron. Soc. Pac., v. 87, no. 520, pp. 917-921; ISSN PASPA
- Country of Publication:
- United States
- Language:
- English
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