Subarcsecond ( ~0\u27:3 x ~0\u27:1) observations of the RX Puppis symbiotic system with the Very Large Array (VLA) have resolved 2 cm continuum emission which deviates from a previously reported circularly symmetric radio distribution. The radio structure is comprised of at least three nearly colinear components. Under the assumption that the strongest feature is coincident with the hot star, the other two features lie 230 and 590 AU distant. These radio features are reminiscent of small-scale radio structure detected toward R Aquarii, another symbiotic star system, and probably represents material ejected from the RX Puppis system at an earlier epoch
© 2022. The Author(s). Published by the American Astronomical Society. This is an open access articl...
Observations of the symbiotic binary R Aquarii environment were obtained with the Very Large Array (...
The study of the formation of massive stars presents complex challenges from both theoretical and ob...
We report evidence for ~1 extended structure in 6 cm continuum emission emanating from the symbioti...
We have obtained the first high-dispersion observations of RX Pup in the wavelength region 1200-2000...
High spectral resolution observations of the peculiar star RX Puppis obtained with the International...
We present an analysis of photometric and spectroscopic observations of the symbiotic binary system ...
Radio continuum observations of the R Aquarii symbiotic star system, using the compact D configurati...
We present an analysis of photometric and spectroscopic observations of the symbiotic binary system ...
We have detected collimated 4.86 GHz (~6 cm) radio continuum emission southwest (SW) of the symbioti...
We present radio and submillimetre observations of the O4I(n)f star ζ Pup, and discuss structure in ...
VLA observations at 6 cm and Lick Observatory optical plates of R Aquarii indicate the existence of ...
High spatial resolution observations (~1 ) of the jet feature associated with the symbiotic variable...
ub-arc second (- 0\u27.\u2715) VLA observations at 2 em have resolved the previously reported 6 em H...
We report Hipparcos observations of a number of binary systems, symbiotic stars and bright long peri...
© 2022. The Author(s). Published by the American Astronomical Society. This is an open access articl...
Observations of the symbiotic binary R Aquarii environment were obtained with the Very Large Array (...
The study of the formation of massive stars presents complex challenges from both theoretical and ob...
We report evidence for ~1 extended structure in 6 cm continuum emission emanating from the symbioti...
We have obtained the first high-dispersion observations of RX Pup in the wavelength region 1200-2000...
High spectral resolution observations of the peculiar star RX Puppis obtained with the International...
We present an analysis of photometric and spectroscopic observations of the symbiotic binary system ...
Radio continuum observations of the R Aquarii symbiotic star system, using the compact D configurati...
We present an analysis of photometric and spectroscopic observations of the symbiotic binary system ...
We have detected collimated 4.86 GHz (~6 cm) radio continuum emission southwest (SW) of the symbioti...
We present radio and submillimetre observations of the O4I(n)f star ζ Pup, and discuss structure in ...
VLA observations at 6 cm and Lick Observatory optical plates of R Aquarii indicate the existence of ...
High spatial resolution observations (~1 ) of the jet feature associated with the symbiotic variable...
ub-arc second (- 0\u27.\u2715) VLA observations at 2 em have resolved the previously reported 6 em H...
We report Hipparcos observations of a number of binary systems, symbiotic stars and bright long peri...
© 2022. The Author(s). Published by the American Astronomical Society. This is an open access articl...
Observations of the symbiotic binary R Aquarii environment were obtained with the Very Large Array (...
The study of the formation of massive stars presents complex challenges from both theoretical and ob...