An Infrared Investigation of Volatiles in Comet 21P/Giacobini-Zinner: Volume 142, Number 2 (1999), pages 482–497

✍ Scribed by H.A. Weaver; G. Chin; D. Bockelée-Morvan; J. Crovisier; T.Y. Brooke; D.P. Cruikshank; T.R. Geballe; S.J. Kim; R. Meier

• Publisher: Elsevier Science
• Year: 2000
• Tongue: English
• Weight: 10 KB
• Volume: 144
• Category: Article
• ISSN: 0019-1035
• DOI: 10.1006/icar.2000.6351

✦ Synopsis

Due to a typesetting error, the last sentence on page 482 was printed incorrectly. It is printed below as it should have appeared:

"C 2 H 6 is depleted by a factor of ∼5 or more compared to its relative abundance in Comets Hale-Bopp (C/1995 O1) and Hyakutake (C/1996 B2); this depletion is similar to that observed for C 2 and C 3 from optical observations of GZ (A'Hearn et al. 1995) and suggests that the formation of volatile carbon-chain molecules was inhibited in GZ."

This erratum is Article ID icar.2000.6351. 203