INVESTIGADORES
CICHOWOLSKI Silvina
artículos
Título:
A DRAO and VLA Investigation of the Environment of WR 130
Autor/es:
CICHOWOLSKI SILVINA; PINEAULT SERGE; ARNAL E. MARCELO; TESTORI J. C.; GOSS, M.; CAPPA CRISTINA E.
Revista:
ASTRONOMICAL JOURNAL
Referencias:
Año: 2001 vol. 122 p. 1938 - 1953
ISSN:
0004-6256
Resumen:
The environment of the Wolf-Rayet (WR) star WR 130 has been studied
using the 21 cm H I line and radio continuum data at 408 and 1420 MHz
obtained with the Dominion Radio Astrophysical Observatory (DRAO)
Synthesis Telescope. In addition, the H110α recombination line and
21 cm H I line were observed using the Very Large Array in the DnC and D
configurations. The Sharpless H II region, Sh 98 (size ~15'), and two OB
stars are observed near the Wolf-Rayet star position. An extended
ring-shaped structure (G68.1+1.1) of size ~20' is observed in the radio
continuum and infrared data. Of four compact radio sources seen
superposed on the ring, one is an H II region of size ~3' (G68.14+0.92),
while the others are probably extragalactic. The spectral index
(Sν~να) of G68.1+1.1 is
α=0.0+/-0.1. The thermal nature of G68.1+1.1 is confirmed by an
analysis of the correlation between the brightness temperature at 21 cm
and the brightness at 60 μm, as observed with IRAS. The DRAO H I data
show an H I bubble in the velocity range -12 to 1 km s-1. The
most striking characteristic of the H I cavity is the excellent
correlation with the radio continuum ring. The WR star is not at the
center of the ring, but in the dense border to the east. This eccentric
position can be explained by a combination of a high spatial velocity
for the star and projection effects. The possible contribution of the OB
stars present in the area is also considered. From our H110α
observations, together with other recombination lines observed in the
area, we deduce a distance of 12 kpc for the compact H II region
G68.14+0.92 and 5 kpc for G68.1+1.1. We conclude that G68.1+1.1 is the
radio counterpart of the optical H II region Sh 98, while G68.14+0.92 is
a chance superposition of a much more distant source. The ionized mass
of the ring is estimated at ~3000 Msolar and the rms electron
density at ~3 cm-3, assuming a homogeneous distribution. A
missing H I mass of 500 Msolar is obtained for the cavity and
an excess H I mass of 1500 Msolar for the shell.