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Erratum: "Measurement of HDCO/H2CO Ratios in the Envelopes of Extremely Cold Protostars in Orion" (2015, ApJ, 814, 31)

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Published 2017 February 14 • © 2017 The American Astronomical Society. All rights reserved.
, , Citation Miju Kang et al 2017 ApJ 836 146 DOI 10.3847/1538-4357/836/1/146

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mjkang@kasi.re.kr

Author affiliations

1 Korea Astronomy and Space Science Institute, 776 Daedeokdaero, Yuseong, Daejeon 305-348, Korea; mjkang@kasi.re.kr

2 Korea University of Science and Technology, Daejeon 305-350, Korea

3 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany

4 Max Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg, Germany

5 National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

6 Department of Astronomical Science, The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

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  1. Received 2017 January 4
  2. Accepted 2017 January 11
  3. Published

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0004-637X/836/1/146

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1. Source Identification

It was found that there are inconsistencies of sources ID numbering between our paper and Furlan et al. (2016). This problem affects only the first column of Table 1 and only the five rows that have both HOPS and PBRS IDs. We provide here the updated Table 1 with the HOPS IDs given by Furlan et al. (2016).

Table 1.  List of Observed Sources

Sourcea R.A. Decl. ${T}_{\mathrm{bol}}$ b ${L}_{\mathrm{bol}}$ b Field
HOPS ID PBRS ID (h:m:s) ($^\circ :^{\prime} :^{\prime\prime} $) (K) (L⊙)  
PBRSs
405 119019 05:40:58.4 −08:05:36.1 34  1.6 L1641
169   05:36:36.0 −06:38:54.0 35  4.5 L1641
398 082005 05:41:29.4 −02:21:17.1 29  1.0 NGC 2024
400 090003 05:42:45.2 −01:16:14.2 36  2.7 NGC 2024
358   05:46:07.2 −00:13:30.9 44 30.6 NGC 2068
373   05:46:30.7 −00:02:36.8 36  5.2 NGC 2068
403 093005 05:46:27.7 −00:00:53.8 31  1.7 NGC 2068
359   05:47:24.8 00:20:58.2 39 12.6 NGC 2068
341   05:47:00.9 00:26:20.8 36  3.6 NGC 2068
404 097002 05:48:07.7 00:33:50.8 33  1.1 NGC 2068
354   05:54:24.1 01:44:20.2 37  7.5 L1622
Non-PBRSsc
164   05:37:00.5 −06:37:10.5 50  0.6 L1641
297   05:41:23.3 −02:17:35.8 46  1.0 NGC 2024
321   05:46:33.2 00:00:02.2 74  4.6 NGC 2068
360   05:47:27.1 00:20:33.1 36  2.2 NGC 2068

Notes.

aIn case there are two source IDs, we use the PBRS ID in the text. bUncertainties of ${T}_{\mathrm{bol}}$ and ${L}_{\mathrm{bol}}$ are ∼15% (Stutz et al. 2013). c ${T}_{\mathrm{bol}}$ and ${L}_{\mathrm{bol}}$ of non-PBRSs are from A. Stutz (2015, private communication) and Furlan et al. (2016).

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10.3847/1538-4357/836/1/146