Other
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008apj...686..748g&link_type=abstract
The Astrophysical Journal, Volume 686, Issue 1, pp. 748-748.
Other
2
Scientific paper
There is an error in the source identification in our KL and M band settings. The results change some quantitative aspects of our results, but do not affect our conclusions. HCN and C2H2 were detected toward the northern component (GV Tau N, or the IRC), rather than the southern component (GV Tau S). This does not affect the K band settings for which we were observing GV Tau S as stated in the paper. Since the K band settings were used to determine N(CO) and abundances were calculated relative to CO, this decreases our calculated abundances by a factor of 2. The values in the following table replace those in Table 2 of the paper. The HCN/CO and C2H2/CO symbols in Figure 6 should also decrease by a factor of 2. Our conclusion that the organics are located close to the host star (IRC rather than GV Tau S) rather than the circumbinary material is unchanged. Our discussion regarding the compositional similarity to chemical models, comets, and other sources is also unaffected.
Brittain Sean D.
Gibb Erika Lynne
Rettig Terrence W.
Van Brunt Kari A.
No associations
LandOfFree
Erratum: ``Warm HCN, C2H2, and CO in the Disk of GV Tau'' (ApJ, 660, 1572 [2007]) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Erratum: ``Warm HCN, C2H2, and CO in the Disk of GV Tau'' (ApJ, 660, 1572 [2007]), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Erratum: ``Warm HCN, C2H2, and CO in the Disk of GV Tau'' (ApJ, 660, 1572 [2007]) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1665751