Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apjs...55..563s&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 55, Aug. 1984, p. 563-570.
Astronomy and Astrophysics
Astronomy
9
Hydrogen Compounds, Interstellar Gas, Line Spectra, Millimeter Waves, Nitrogen Compounds, Submillimeter Waves, Astronomical Models, Radicals, Radio Astronomy
Scientific paper
The identification of interstellar molecular species via the detection of one spectral line has recently become subject to close scrutiny. The radical HNO falls into the class of interstellar molecules identified in this manner. To corroborate this identification, observation of additional spectral lines is necessary. In this paper, laboratory millimeter and submillimeter wave spectra of both HNO and DNO are reported in the frequency region 150-500 GHz. Based on these spectral line measurements, models for HNO and DNO have been constructed to yield accurate frequencies for all rotational transitions of these species below 500 GHz involving J values smaller than 10. The spectral lines can be utilized by radio astronomers to confirm the identification of interstellar HNO and to search for interstellar DNO.
de Lucia Frank C.
Helminger Paul
Herbst Eric
Plummer Grant M.
Sastry V. L. N. K.
No associations
LandOfFree
Laboratory millimeter and submillimeter spectra of HNO and DNO does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Laboratory millimeter and submillimeter spectra of HNO and DNO, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Laboratory millimeter and submillimeter spectra of HNO and DNO will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1674957