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Observations of HNO

Published online by Cambridge University Press:  07 August 2017

L. E. Snyder ,
J. M. Hollis ,
L. M. Ziurys  and
Y.-J. Kuan
L. E. Snyder
Affiliation:
Astronomy Dept., Univ. of Illinois;
J. M. Hollis
Affiliation:
Space Data & Computing Div., NASA/GSFC;
L. M. Ziurys
Affiliation:
Chemistry Dept., Arizona State Univ.
Y.-J. Kuan
Affiliation:
Astronomy Dept., Univ. of Illinois;

Abstract

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Interferometric observations of the HNO 3.68 mm line in Sgr B2 show clumping and some distribution similarities with HNCO. A search for the HNO 1.23 mm line with the NRAO 12-m telescope was unsuccessful.

Type
Quiescent Clouds and Regions of Star Formation
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 187 - 188
Copyright
Copyright © Kluwer 1992 

References

REFERENCES

Hollis, J. M., Snyder, L. E., Ziurys, L. M., and McGonagle, D. (1991) ‘Interstellar HNO:confirming the identification’, in Haschick, A. D. and Ho, P. T. P. (eds), Skylines, ASP Conference Series 16, San Francisco, pp. 407–12.Google Scholar
Snyder, L.E., Kuan, Y.-J., and Pratap, P. (1991) ‘Millimeter wavelength molecular maps of the clumped gas around Sgr B2(OH)’, Ibid., pp. 191–6.Google Scholar