Display data from paper

Select data type:

FUR03 - Water Maser Survey toward Low-Mass Young Stellar Objects in the Northern Sky with the Nobeyama 45 Meter Telescope and the Very Large Array

Short title: Furuya et al. (2003)
Authors: Furuya, Ray S.Kitamura, YoshimiWootten, AlwynClaussen, Mark J.Kawabe, Ryohei
Journal: The Astrophysical Journal Supplement Series, Volume 144, Issue 1, pp. 71-134.
Bibcode:

Target type: YSO

Abstract
We give a detailed presentation of all the data from a multiepoch 22 GHz H₂O maser survey mainly toward low-mass young stellar objects (YSOs) using the Nobeyama 45 m telescope and the Very Large Array (VLA). Our major results are already published (our Paper I). The Nobeyama survey is the first complete H₂O maser survey toward known Class 0 sources in the northern sky (delta>-35^deg) and is one of the most sensitive surveys ever performed. The survey was conducted from 1996 May through 1999 March over 32 periods. A total of 606 observations were carried out toward 173 YSOs, including 36 unknown luminosity sources, and toward 31 preprotostellar cores (PPSCs) in the Ophiuchus star-forming region. We detected 149 spectra toward 39 YSOs and zero spectra toward the 31 PPSCs. Subsequent to the Nobeyama survey, we performed a follow-up interferometric survey with the VLA in order to associate 19 maser sources detected by the 45 m telescope with individual YSOs. In this paper we compile properties of 142 YSOs together with their H₂O maser activity. On the basis of this data set, we use properties of water maser emission as a probe of jet phenomena in low-mass stars.	Comments: Interferometry data is not entered yet

Abstract

We give a detailed presentation of all the data from a multiepoch 22 GHz H₂O maser survey mainly toward low-mass young stellar objects (YSOs) using the Nobeyama 45 m telescope and the Very Large Array (VLA). Our major results are already published (our Paper I). The Nobeyama survey is the first complete H₂O maser survey toward known Class 0 sources in the northern sky (delta>-35^deg) and is one of the most sensitive surveys ever performed. The survey was conducted from 1996 May through 1999 March over 32 periods. A total of 606 observations were carried out toward 173 YSOs, including 36 unknown luminosity sources, and toward 31 preprotostellar cores (PPSCs) in the Ophiuchus star-forming region. We detected 149 spectra toward 39 YSOs and zero spectra toward the 31 PPSCs. Subsequent to the Nobeyama survey, we performed a follow-up interferometric survey with the VLA in order to associate 19 maser sources detected by the 45 m telescope with individual YSOs. In this paper we compile properties of 142 YSOs together with their H₂O maser activity. On the basis of this data set, we use properties of water maser emission as a probe of jet phenomena in low-mass stars.

Comments:
Interferometry data is not entered yet

Download as: Table (CSV)
View as list of objects

Detection table from Furuya et al. (2003)

Export table to csv

Hide / Show individual components

Non-detection table from Furuya et al. (2003)