Jy. Shin et al., THE SHELL OF QU-VULPECULAE AT 2.2 MICRONS, H-ALPHA, AND 3.6 CENTIMETERS, The Astronomical journal (New York), 116(4), 1998, pp. 1966-1970
Observations of the classical nova QU Vul (1984) were carried out in t
he infrared, optical, and radio regimes between days 3791 and 4262 aft
er discovery. For the first time a spatial extension of the shell arou
nd QU Vul could be unambiguously established from our IR and optical o
bservations. At. 2.2 mu m, a shell size of about 0.'' 8 was found, whi
ch corresponds to a linear diameter of (4.5 +/- 0.4) x 10(16) cm on da
y 4124 assuming QU Vul is 3.6 kpc distant. The mass of the shell is (4
+/- 1.5) x 10(-4) M-. with the assumption that a free-free emission p
rocess is the dominant emission mechanism in the shell. This shell mas
s is larger than found for any nova.