Methylidynium, CH+, was one of the first molecules to be identified
in space. Its electronic A 1Π X
1Σ spectrum was detected in the lowest R(0)
transition of the three v =
0 0, 1 0, and 2 0
vibrational bands at 423.257, 395.771, and 374.530 nm, respectively:
A. E. Douglas and G.Herzberg,
Note on CH+ in Interstellar Space and in the Laboratory.
Astrophys. J. 94, 381 (1941).
The first two lines were detected toward ξ Per, χ2 Ori, and 55 Cyg, the very first one also toward χ Aur by
T. Dunham, Jr.,
Interstellar Neutral Potassium and Neutral Calcium
Publ. Astron. Soc. Pac. 49, 2628 (1937).
As mentioned there, these lines were also observed by:
W. S. Adams,
Some Results with the COUDÉ Spectrograph of the Mount Wilson Observatory
Astrophys. J. 93, 1123 (1941);
He reportedly also observed the third line.
The detection of its pure rotational spectrum toward in the planetary
nebula NGC 7027 was reported by
J. Cernicharo, X.-W. Liu, E. González-Alfonso, P. Cox, M. J. Barlow, T. Lim, and B. M. Swinyard,
Discovery of Far-Infrared Pure Rotational Transitions of CH+ in NGC 7027
Astrophys. J. 483, L65L68 (1997).
More recently, interstellar methylidynium has been observed for the first time
in high resolution and in absorption towards the star-forming region G10.6-0.4.
Actually, as observation of the J = 1 0
transition of 12CH+ is hampered by a terrestrial
O2 line, 13CH+ was observed instead:
E. Falgarone, T. G. Phillips, and J. C. Pearson,
First Detection of 13CH+ (J = 1 0)
Astrophys. J. 634, L149L152 (2005).
Please note that the inferred rest-frequency is incorrect. Two alternative rest frequencies were proposed of which the higher one is quite appropriate.
The J = 1 0 transition of 12CH+
has been detected with the Herschel satellite in emission toward the
Orion Bar by
E. Habart, E. Dartois, A. Abergel, et al.,
SPIRE Spectroscopy of the Prototypical Orion Bar Photodissociation Region
Astron. Astrophys. 518, Art. No. L116 (2010);
D. A. Naylor, E. Dartois, E. Habart,
First Detection of the Methylidyne Cation (CH+) Fundamental Rotational Line with the Herschel/SPIRE FTS
Astron. Astrophys. 518, Art. No. L117 (2010).
The latter work also describes the observation of this transition in absorption toward two compact HII regions.
E. Falgarone, V. Ossenkopf, M. Gerin, et al. observed
Strong CH+ J = 1 0 Emission and Absorption in DR21
Astron. Astrophys. 518, Art. No. L118 (2010).
These authors were the first to use the correct rest frequency of 835137.5 MHz.
Higher-J transitions of CH+ were also detected with the PACS instrument
on board of the Herschel satellite in the disc around a Herbig Be star by:
W-F. Thi, F. Menard, G. Meeus, C. Martin-Zaidi, P. Woitke, E. Tatulli, M. Benisty, I. Kamp, I. Pascucci, C. Pinte, C. A. Grady, S. Brittain, G.J. White, C. D. Howard, G. Sandell, C. Eiroa,
Detection of CH+ Emission from the Disc around HD 100546
Astron. Astrophys. 530, Art. No. L2 (2011).