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Table 2
Transitions of TiO covered by APEX, Herschel, and ALMA.
Isoto- | Jup → Jlow, | ν | Err(ν)a | S μ 2 | E u | Dates of | Vis. | Flux (1σ) |
pologue | multiplet ΔΩ | (MHz) | (km s-1) | (Debye2) | (K) | observation | phase | (Jy km s-1) |
|
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APEX | ||||||||
|
||||||||
48TiO | 7 → 6, Δ1 | 221 580.45 | 0.05 | 153.0 | 41.0 | 3–20 Dec. 2013, 1–7 Aug. 2016 | 0.5/0.35 | 0.89 (0.21) |
7 → 6, Δ2 | 224 138.74 | 0.03 | 143.4 | 180.7 | 3–20 Dec. 2013, 1–7 Aug. 2016 | 0.5/0.35 | <0.60 | |
11 → 10, Δ3 | 355 623.35 | 0.04 | 227.2 | 386.2 | 30 Jun.–6 Jul. 2014 | 0.0 | 3.14 (0.73) | |
13 → 12, Δ3 | 420 224.14 | 0.04 | 274.7 | 425.0 | 13–14 Aug. 2013 | 0.1 | 9.67 (1.81) | |
15 → 14, Δ3 | 484 795.99 | 0.06 | 321.4 | 470.0 | 1–8 Jul. 2014 | 0.0 | 8.66 (1.50) | |
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Herschel | ||||||||
|
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48TiO | 18 → 17, Δ1 | 569 537.72 | 0.13 | 400.3 | 258.2 | 19 Jul. 2010 | 0.7 | <22.57 |
18 → 17, Δ2 | 575 979.23 | 0.13 | 396.5 | 400.4 | 19 Feb. 2010 | 0.3 | <21.97 | |
20 → 19, Δ3 | 646 070.05 | 0.26 | 436.2 | 609.6 | 20 Jul. 2010 | 0.7 | <28.20 | |
25 → 24, Δ3 | 807 067.03 | 0.75 | 549.9 | 787.7 | 4 Feb. 2010 | 0.2 | <30.80 | |
29 → 28, Δ3 | 935 619.31 | 1.48 | 640.2 | 958.1 | 10 Aug. 2011, 28 Jan. 2012b | 0.9/0.4 | <222.89 | |
34 → 33, Δ3 | 1 095 946.06 | 2.98 | 752.8 | 1205.7 | 20 Jul. 2010 | 0.7 | 65.25 (18.31) | |
|
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ALMA | ||||||||
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50TiO | 11 → 10, Δ1 | 344 722.34 | >0.02 | 240.9 | 97.8 | 12–15 Jun. 2014 | 1.0 | 0.31 (0.02) |
48TiO | 21 → 20, Δ3 | 678 293.80 | 0.33 | 459.0 | 642.1 | 16 Jun. 2014 | 1.0 | 16.36 (1.00) |
46TiO | 11 → 10, Δ2 | 355 975.66 | >0.02 | 239.8 | 240.2 | 21 Jul. 2015 | 0.2 | 0.54 (0.02) |
47TiO | 11 → 10, Δ3 | 357 526.69 | >0.04 | 228.4 | 386.8 | 21 Jul. 2015 | 0.2 | <0.33 (0.02) |
48TiO | 11 → 10, Δ3 | 355 623.35 | 0.04 | 227.2 | 386.2 | 21 Jul. 2015 | 0.2 | 4.44 (0.03) |
50TiO | 11 → 10, Δ1 | 344 722.34 | >0.02 | 240.9 | 97.8 | 21 Jul. 2015 | 0.2 | 0.39 (0.02) |
Notes. Spectroscopic data for e and f parity components were combined. The flux is given with a 1σ error in the parenthesis. Upper limits on flux have a 3σ significance.
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