Position: 19 07 36.90 +12 31 26.2 Akimasa Nakamura 19 07 36.92 +12 31 26.5 Nick James (11 GSC V1.2 stars) 19 07 36.89 +12 31 26.5 Gianluca Masi (6 USNO A2.0 stars)
K. Ayani and T. Kawabata at Bisei Astronomical Observatory (BAO), Okayama, Japan, obtained a low resolution spectrum (470-680nm) of the nova on July 14.6 UT with BAO 1.01-m telescope. Strong, broad H-alpha and H-beta lines are visible. The H-alpha line has a FWHM of about 3400 km/s and a equivalent width of about 50 nm.
Patrick Schmeer reported on VSNET that there is no prenova candidate visible on the POSS to a limiting magnitude of 20.