Hostname: page-component-8448b6f56d-qsmjn Total loading time: 0 Render date: 2024-04-23T11:01:40.876Z Has data issue: false hasContentIssue false
  • English
  • Français

VLA observations of H2O and OH (1612 MHz) maser emission towards OH 231.8+4.2

Published online by Cambridge University Press:  03 August 2017

Yolanda Gómez  and
Luis F. Rodríguez
Yolanda Gómez
Affiliation:
Instituto de Astronomía, UNAM, Apdo. Postal 3-72 (Xangari), 58089 Morelia, Michoacán, México
Luis F. Rodríguez
Affiliation:
Instituto de Astronomía, UNAM, Apdo. Postal 3-72 (Xangari), 58089 Morelia, Michoacán, México

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present Very Large Array (VLA) observations of H2O and OH (1612 MHz) maser emission toward the protoplanetary nebula OH 231.8+4.2. The H2O observations show two features at VLSR of 23.1 and 44.5 km s−1, coinciding in position within error with the SiO (v=1; J=2−1) maser position from Sánchez Contreras et al. (2000). The H2O and SiO masers are most likely tracing the position of QX Pup, the Mira near the center of OH 231.8+4.2. This position is, however, clearly offset by ∼1 from the axis of the bipolar outflow traced by the OH maser emission. These results suggest the presence of a binary system: one invisible star powering the bipolar outflow and the other, the Mira star QX Pup, associated with the H2O and SiO masers. This scenario requires that the two stars have evolved at very similar rates.

Type
Part 3. Protoplanetary Nebulae
Information
Symposium - International Astronomical Union , Volume 206: Cosmic Masers: From Protostars to Blackholes , 2002 , pp. 348 - 351
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

Bowers, P. F. & Morris, M. 1984, ApJ, 276, 646 Google Scholar
Cohen, M. 1981, PASP, 93, 288 Google Scholar
Cohen, M., Dopita, M. A., Schwartz, R. D., & Tielens, A. 1985, ApJ, 297, 702 Google Scholar
Feast, M. W., Catchpole, R. M., Whitelock, P. A., Roberts, G., Jones, J. S., and Carter, B. S. 1983, MNRAS, 203, 1207 CrossRefGoogle Scholar
Gómez, Y., Moran, J.M., & Rodríguez, L.F. 1990, RevMexA&A, 20, 55 Google Scholar
Kastner, J.H., Zuckerman, B., Becklin, E. E., McLean, I., & Gatley, I. 1992, ApJ, 398, 552 CrossRefGoogle Scholar
Kastner, J.H., Weintraub, D.A., Merril, K.M. & Gatley, I. 1998, AJ, 116, 1412 Google Scholar
Lewis, B. M. 1989, AJ, 338, 234 CrossRefGoogle Scholar
López, J. A., Meaburn, J., Rodríguez, L. F., Vázquez, R., Steffen, W., & Bryce, M. 2000, ApJ, 538, 233 CrossRefGoogle Scholar
Morris, M., Bowers, P. F., & Turner, B. E. 1982, ApJ, 259, 625 Reipurth, B. 1987, Nature, 325, 787 Google Scholar
Sánchez Contreras, C., Bujarrabal, V., & Alcolea, J. 1997, A&A, 327, 689 Google Scholar
Sánchez Contreras, C., Bujarrabal, V., Miranda, L.F., et al. 2000, A&A, 355, 1103 Google Scholar
Shure, M., Sellgren, K., Jones, T. J., & Klebe, D. 1995, AJ, 109, 721 Miranda, L. F., & Fernández-Figueroa, M. J. 2000, A&A, 355, 1103 CrossRefGoogle Scholar
Zijlstra, A. A. et al. 2001, MNRAS, 322, 280 Google Scholar