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Table 2

Frequency, absorption oscillator strength, and detection rates of observed hydrogen millimeter recombination lines.

mm-RRL Rest frequency Absorption Number of Number of Detection rateb
transition (MHz) oscillator strength* observed sources detected sourcesa

H −− 976 178 18 ± 1
H39α 106 737.4 7.725489 385 58 15 ± 2
H40α 99 023.0 7.916287 366 57 16 ± 2
H41α 92 034.4 8.107084 972 146c 15 ± 1
H42α 85 688.4 8.297880 973 136 14 ± 1

H −− 976 65 7 ± 1
H48β 111 885.1 1.342709 366 20 5 ± 1
H49β 105 301.9 1.369046 385 26 7 ± 1
H50β 99 225.2 1.395383 366 28 8 ± 1
H51β 93 607.3 1.421720 366 28 8 ± 1
H52β 88 405.7 1.448056 971 47 5 ± 1

H −− 389 23 6 ± 1
H55γ 109 536.0 0.482179 366 17 5 ± 1
H56γ 103 914.8 0.490287 385 17 4 ± 1
H57γ 98 671.9 0.498395 366 18 5 ± 1
H58γ 93 775.9 0.506503 366 19 5 ± 1
H60γ 84 914.4 0.522718 385 15 4 ± 1

H −− 389 22 6 ± 1
H60δ 110 600.7 0.230388 366 9 2 ± 1
H61δ 105 410.2 0.233881 385 9 2 ± 1
H62δ 100 539.6 0.237374 385 11 3 ± 1
H63δ 95 964.6 0.240867 366 10 3 ± 1
H64δ 91 663.1 0.244359 384 11 3 ± 1
H65δ 87 615.0 0.247852 383 7 2 ± 1

Notes. The H, H, and H mm-RRLs are only detected toward clumps where the peak intensities of H mm-RRLs are brighter than 0.24, 0.62, and 0.54 Jy, respectively. Column 1 is mm-RRLs increasing transition, in Cols. 2 and 3 we give the numbers of observed and detected sources, respectively. The last column shows the detection rates. Line parameters and rms levels of the stacked and individual transitions are available in electronic form at the CDS.

(†)

Mopra 22 m covered only these three transitions.

(a)

A detection requires a stacked signal above 3σ.

(b)

The statistical errors of detection rates are obtained assuming binomial statistics.

(c)

Some H41α spectra are located at an edge or beyond observed band width.

Reference.

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