SIMBAD references

2013ApJ...771L..10C - Astrophys. J., 771, L10 (2013/July-1)

Detection of the ammonium ion in space.

CERNICHARO J., TERCERO B., FUENTE A., DOMENECH J.L., CUETO M., CARRASCO E., HERRERO V.J., TANARRO I., MARCELINO N., ROUEFF E., GERIN M. and PEARSON J.

Abstract (from CDS):

We report on the detection of a narrow feature at 262816.73 MHz toward Orion and the cold prestellar core B1-bS which we attribute to the 10-00 line of the deuterated ammonium ion, NH3D+. The observations were performed with the IRAM 30 m radio telescope. The carrier has to be a light molecular species as it is the only feature detected over 3.6 GHz of bandwidth. The hyperfine structure is not resolved, indicating a very low value for the electric quadrupolar coupling constant of nitrogen which is expected for NH3D+ as the electric field over the N nucleus is practically zero. Moreover, the feature is right at the predicted frequency for the 10-00transition of the ammonium ion, 262817±6 MHz (3σ), using rotational constants derived from new infrared data obtained in our laboratory in Madrid. The estimated column density is (1.1±0.2)x1012/cm2. Assuming a deuterium enhancement similar to that of NH2D, we derive N(NH44) ≃ 2.6x1013/cm2, i.e., an abundance for ammonium of a few 10–11.

Abstract Copyright:

Journal keyword(s): ISM: abundances - ISM: individual: B1-bS - ISM: molecules - line: identification - molecular data

Simbad objects: 3

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