Lf. Rodriguez et B. Reipurth, VLA DETECTION OF THE EXCITING SOURCES OF HH-34, HH-114, AND HH-199, Revista Mexicana de Astronomia y Astrofisica, 32(1), 1996, pp. 27-33
We present sensitive VLA observations at 3.6-cm of four Herbig-Haro fi
elds: HH 34, HH 114, HH 199, and RH 212. In all fields but the last we
detect radio sources that are probably associated with the exciting s
ource of the region. In the case of HH 34, our detection of a radio co
unterpart supports the notion that newborn stars which are actively pr
oducing RH flows generally emit in the cm radio continuum at levels th
at are detectable with a moderately long (a few hours) integration mad
e with the VLA. In the HH 114 field, we detect independent sources ass
ociated with both an IRAS source and a millimeter object in the region
. Our present observations cannot favor either of the sources as the d
ominant exciting object in the region. Finally, in HH 199 we detect a
source that could be a thermal jet or an unresolved radio binary and t
hat is associated with the IRAS source in the field.