Whelan, Emma and Ray, T.P. and Podio, L. and Bacciotti, F. and Randich, S.
(2014)
Erratum: "Classical T Tauri-like Ouflow Activity in the Brown Dwarf Mass Regime" (2009, ApJ, 706, 1054)*.
Astrophysical Journal, 788 (194).
ISSN 0004-637X
Abstract
Figures 3–11 have an error in that the direction of the offsets should be reversed. Thus, in the spectro-astrometric plots, positive offsets are toward the top of the figure and negative offsets toward the bottom. In the position–velocity diagram shown in Figure 8, positive offsets are toward the left and negative toward the right. The result of this correction is that the orientations of the blueshifted and redshifted lobes of the outflows are now reversed. Thus, for ISO-Cha1 217 the blueshifted flow is the in northeast quadrant with a position angle (P.A.) of 20° and the redshifted flow is in the southwest quadrant (see Figure 2). Similarly, for ISO-Oph 32, the blueshifted flow now lies in the northeast quadrant with a P.A. of 60°. Table 3 has been updated accordingly.
Item Type: |
Article
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Additional Information: |
This is an erratum for the article 2009 ApJ 706 1054 |
Keywords: |
ISM: jets and outflows; stars: formation; stars: low-mass, brown dwarfs; |
Academic Unit: |
Faculty of Science and Engineering > Experimental Physics |
Item ID: |
9916 |
Identification Number: |
https://doi.org/10.1088/0004-637X/788/2/194 |
Depositing User: |
Emma Whelan
|
Date Deposited: |
13 Sep 2018 14:33 |
Journal or Publication Title: |
Astrophysical Journal |
Publisher: |
American Astronomical Society |
Refereed: |
Yes |
URI: |
|
Use Licence: |
This item is available under a Creative Commons Attribution Non Commercial Share Alike Licence (CC BY-NC-SA). Details of this licence are available
here |
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