SIMBAD references

2013ApJ...778L...1G - Astrophys. J., 778, L1 (2013/November-3)

Laboratory measurements and tentative astronomical identification of H2NCO+.

GUPTA H., GOTTLIEB C.A., LATTANZI V., PEARSON J.C. and McCARTHY M.C.

Abstract (from CDS):

The rotational spectrum of H2NCO+, the ground-state isomer of protonated HNCO, has been measured in a molecular beam in the centimeter band with a Fourier transform microwave spectrometer and in a low-pressure laboratory discharge in absorption in the millimeter band. Spectroscopic constants, including the nitrogen-14 hyperfine coupling constant, derived from 30 a-type transitions between 20 and 367 GHz with J ≤ 18 and Ka ≤ 3 allow the principal rotational transitions to be calculated to 1 km/s or better in equivalent radial velocity well into the far IR. Two low-lying rotational transitions of H2NCO+ in the centimeter band (0_0, 0–10, 1_ and 1_1, 0–21, 1_) were tentatively identified in absorption in the PRIMOS spectral line survey of Sgr B2(N) with the Green Bank Telescope. The lines of H2NCO+ arise in a region of the Sgr B2(N) halo whose density is low (n < 1x104/cm3). The derived column density of (6-14)x1011/cm2 implies that the fractional abundance is ∼10–12. Owing to the ubiquity of HNCO in galactic molecular clouds, H2NCO+ is a good candidate for detection in sources spanning a wide range of physical conditions.

Abstract Copyright:

Journal keyword(s): ISM: molecules

Simbad objects: 3

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2013ApJ...778L...1G and select 'bookmark this link' or equivalent in the popup menu


2020.01.24-23:31:21

© Université de Strasbourg/CNRS

    • Contact