Abstract
We present a study of the structure and dynamics of the star-forming region B1-IRS (IRAS 03301+3057) using the properties of different molecules at high angular resolution (∼4″). We have used VLA observations of NH3, CCS, and H2O masers at 1 cm. CCS emission shows three clumps around the central source, with a velocity gradient from red to blue-shifted velocities towards the protostar, probably due to the interaction with outflowing material. Water maser emission is elongated in the same direction as a reflection nebula detected at 2 μm by 2MASS, with the maser spots located in a structure of some hundreds of AU from the central source, possibly tracing a jet. We propose a new outflow model to explain all our observations, consisting of a molecular outflow near the plane of the sky. Ammonia emission is extended and anticorrelated with CCS. We have detected for the first time this anticorrelation at small scales (1400 AU) in a star-forming region.
Similar content being viewed by others
References
Furuya, R.S., Kitamura, Y., Wootten, H.A., Claussen, M.J. and Kawabe, R.: 2001, ApJ 559, L143.
Hirano, N., Kameya, O., Mikami, H., Saito, S., Umemoto, T. and Yamamoto, S.: 1997, ApJ 478, 631.
Kuiper, T.B.H., Langer, W.D. and Velusamy, T.: 1996, ApJ 468, 761.
Rodríguez, L.F., Moran, J.M., Gottlieb, E.W. and Ho, P.T.P.: 1980, ApJ 235, 845.
Saito, S., Kawaguchi, K., Yamamoto, S., Ohishi, M., Suzuki, H. and Kaifu, N.: 1987, ApJ 317, L115.
Suzuki, H., Yamamoto, S., Ohishi, M., Kaifu, N., Ishikawa, S., Hirahara, Y. and Takano, S.: 1992, ApJ 392, 551.
Velusamy, T., Kuiper, T.B.H. and Langer, W.D.: 1995, ApJ 451, L75.
Yamamoto, S., Mikami, H., Saito, S., Kaifu, N., Ohishi, M. and Kawaguchi, K.: 1992, PASJ 44, 459.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
De Gregorio-Monsalvo, I., Chandler, C.J., Gómez, J.F. et al. High-Resolution Observations in B1-IRS: Ammonia, Ccs and Water Masers. Astrophys Space Sci 295, 65–70 (2005). https://doi.org/10.1007/s10509-005-3661-6
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/s10509-005-3661-6