A search for cool molecular gas in GK Persei and other classical novae

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Volume 659 (March 2022)

A&A, 659 (2022) A109

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Table 8

Novae observed with the SMA.

Object	Alter. name	RA (J2000)	Dec (J2000)	Obs. dates	Beam_CO	Beam_HCN	rms_CO	rms_HCN
				2017	(′′)	(′′)	(mJy/beam)
NQ Vul	Nova Vul 1976	19:29:14.75	+20:27:59.63	19,20 Jun.; 5,9 Jul.	3.7 × 3.0	3.4 × 2.3	13.9	15.2
LW Ser	Nova Ser 1978	17:51:50.89	–14:43:50.60	5 Jul.	4.0 × 3.0	2.6 × 2.1	14.7	36.7
V2676 Oph	Nova Oph 2012	17:26:07.08	–25:51:45.40	19 Jun.	4.5 × 3.1	2.9 × 2.0	9.6	27.1
V3662 Oph	Nova Oph 2017	17:39:46.08	–24:57:55.50	20 Jun.	4.4 × 3.1	2.8 × 2.0	13.2	31.9

Notes. Beam sizes are given as FWHMs at the natural weighting of visibilities. The rms values, rms_CO and rms_HCN, are specified for a spectral bin of 30 km s⁻¹ near the rest frequencies of CO(2–1) and HCN(4–3), respectively.

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