A Search for Interstellar CH 2 D

• Published in: Proceedings of the International Astronomical Union Vol. 4; no. S251; pp. 33 - 34
• Main Authors: Wootten, Alwyn, Turner, Barry E.
• Format: Journal Article
• Language: English
• Published: 01.02.2008
• ISSN: 1743-9213; 1743-9221
• DOI: 10.1017/S1743921308021121

Abstract We report on a search for interstellar CH 2 D + . Four transitions occur in easily accessible portions of the spectrum; we report on emission at the frequencies of these transitions toward high column density star-forming regions. While the observations can be interpreted as being consistent with a detection of the molecule, further observations will be needed to secure its identification. The CH 2 D + rotational spectrum has not been measured to high accuracy. Its lines are weak, as the dipole moment induced by the inclusion of deuterium in the molecule is small. Astronomical detection is favored by observations toward strongly deuterium-fractionated sources. However, enhanced deuteration is expected to be most significant at low temperatures. The sparseness of the available spectrum and the low excitation in regions of high fractionation make secure identification of CH 2 D + difficult. Nonetheless, owing to the importance of CH 3 + to interstellar chemistry, and the lack of rotational transitions of that molecule owing to its planar symmetric structure, a measure of its abundance would provide key data to astrochemical models.