(sorry for the late relay) Date: Thu, 2 Dec 1999 21:11:35 +0100 (CET) From: Ulisse Munari <ulisse@ulisse.pd.astro.it> Subject: [vsnet-alert 0] Asiago spectroscopy of Nova Aql 1999 N.2 The following message has been sent to CBAT regards Ulisse Munari "1 nm/pix, 340-950 nm range spectra of Nova Aql 1999 N.2 have been obtained on Dec. 2.71, 1999 with the B&C+CCD spectrograph on the Asiago 1.22 m telescope. The Balmer hydrogen series is in emission with a P-Cyg profile. The Halpha emission component has a 1300 km/sec FWHM, the absorption component is centered at -1850 km/sec from the emission one. FeII emission lines multiplet N.42 at 492, 502 and 517 nm and OI 777 nm are visible in emission with a P-Cyg profile too. Moro D., Pizzella A. and Munari U., Asiago Astrophysical Observatory, Italy"