| Issue |
A&A
Volume 549, January 2013
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 1 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201219728e | |
| Published online | 20 December 2012 | |
Estimating distance, pressure, and dust opacity using submillimeter observations of self-gravitating filaments (Corrigendum)
Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, ON M5S3H8, Canada
e-mail: fischera@cita.utoronto.ca
Key words: methods: observational / techniques: photometric / ISM: clouds / dust, extinction / ISM: structure / errata, addenda
The formula for the flux density per unit length (Eq. (8) in the paper of Fischera & Martin 2012) contained the product δην. Since the notation ην already incorporates δ implicitly, the correct form is 
(8)
This is a notational error, not used in our calculations, and so it does not affect any of the results.
References
- Fischera, J., & Martin, P. G. 2012, A&A, 547, A86 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© ESO, 2012
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