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Table 1

Millimeter molecular line observations of CB 26(a) and summary of observing parameters.

Line Frequ. [GHz] Tel. Year uv radius range [m] Bandw. [km s−1] υchan [km s−1] Primary HPBW [arcsec] Synthesized HPBW (PA) [arcsec (deg)] 1σ rms [mJy beam−1]
12CO(2–1) 230.538 PdBI(a) 2005,2009 18 (b)–753 14 0.20 21.9 0.53 × 0.47 (6.9)(c) 8
13CO(1–0) 110.201 OVRO 2001 12-478 4.8 0.15 45.7 1.20 × 0.88 (91.7) 35
HCO+ (1–0) 89.189 PdBI(a) 2005 17 (b)–175 12.8 0.20 56.5 3.74 × 3.38 (100.3) 7
H13CO+ (1–0) 86.754 PdBI (a) 2008,2009 20 (b)–175 7 0.50 58.1 4.09 × 2.26 (114.6) 5
HCO+ (3–2) 267.558 SMA 2006 11–192 29 0.23 18.8 1.37 × 1.34 (39.0) 150

Notes. (a)The phase center was at α2000 = 04h59m50.74s, δ2000 = 52°04′43.80″. (b)Plus zero-spacing observations with the IRAM 30m telescope (see Sect. 2.2). (c)Natural uv-weighting. We also produced maps with robust uv-weighting (HPBW 0.48 × 0.42″) and a tapered (smoothed) map (HPBW 1.08 × 0.92″, see Sect. 3.3).

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