Upper limits for CO in the old Galactic novae NQ Vulpeculae, QU Vulpeculae, and Nova Vulpeculae 1987 from IRAM observations

Details Upper limits for CO in the old Galactic novae NQ Vulpeculae, QU Vulpeculae, and Nova Vulpeculae 1987 from IRAM observations Upper limits for CO in the old Galactic novae NQ Vulpeculae, QU Vulpeculae, and Nova Vulpeculae 1987 from IRAM observations

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...392l..59s&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 392, no. 2, June 20, 1992, p. L59-L61. Research supported by NATO

Astronomy and Astrophysics

Astronomy

4

Cataclysmic Variables, Emission Spectra, Molecular Clouds, Novae, Radio Astronomy, Carbon Monoxide, Carbon 12, Interstellar Matter, Iue

Scientific paper

Three Galactic novae were observed with the IRAM 30 M telescope at
(C-12)O J = 1 - 0 and J = 2 - 1. No evidence for the previously reported
emission in NQ Vul is found and strong upper limits are derived for
possible CO emission in QU Vul and Nova Vul 1987. There is no evidence
for extensive cold molecular material surrounding old novae.

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