Correlation between Infrared Colors and Intensity Ratios of SiO Maser Lines
arXiv:0706.0945 · doi:10.1086/520825
Abstract
We present the results of SiO millimeter-line observations of a sample of known SiO maser sources covering a wide dust-temperature range. A cold part of the sample was selected from the SiO maser sources found in our recent SiO maser survey of cold dusty objects. The aim of the present research is to investigate the causes of the correlation between infrared colors and SiO maser intensity ratios among different transition lines. In particular, the correlation between infrared colors and SiO maser intensity ratio among the J=1-0 v=1, 2, and 3 lines are mainly concerned in this paper. We observed in total 75 SiO maser sources with the Nobeyama 45m telescope quasi-simultaneously in the SiO J=1-0 v=0, 1, 2, 3, 4 and J=2-1 v=1, 2 lines. We also observed the sample in the 29SiO J=1-0 v=0 and J=2-1 v=0, and 30SiO J=1-0 v=0 lines, and the H2O 6(1,6)-5(2,3) line. As reported in previous papers, we confirmed that the intensity ratios of the SiO J=1-0 v=2 to v=1 lines clearly correlate with infrared colors. In addition, we found possible correlation between infrared colors and the intensity ratios of the SiO J=1-0 v=3 to v=1&2 lines. Two overlap lines of H2O (i.e., 11(6,6) nu_2=1 -> 12(7,5) nu_2=0 and 5(0,5) nu_2=2 -> 6(3,4) nu_2=1) might explain these correlation if these overlap lines become stronger with increase of infrared colors, although the phenomena also might be explained by more fundamental ways if we take into account the variation of opacity from object to object.
arXiv comment49 pages, 7 figures, 3 tables, accepted for publication in ApJ. Full resolution version available at http://www.asiaa.sinica.edu.tw/~junichi/paper/
References in corpus (15)
- Large Synoptic Survey Telescope: Overview
- A movie of a star: multi-epoch VLBA imaging of the SiO masers towards the Mira variable TX Cam
- High resolution observations of SiO masers: comparing the spatial distribution at 43 and 86 GHz
- 86 GHz SiO maser survey of late-type stars in the Inner Galaxy. I. Observational data
- SiO Maser Survey of IRAS Sources in the Inner Galactic Disk
- SiO Maser Survey of Cold IRAS Sources
- SiO masers in TX Cam: Simultaneous VLBA observations of two 43 GHz masers at four epochs
- SiO Maser Survey of the Inner Bar of the Galactic Bulge
- Detections of SiO and HO Masers in the Bipolar Nebula IRAS 19312+1950
- Period Measurement of AGB Stars in the Outer Galactic Disk
- SiO Maser Survey toward the Inner Galactic Disk: 40 < l < 70 and |b| < 10
- Study of the Bipolar Nebula IRAS 19312+1950. I. Mapping Observations
- BIMA Array Observations of the Highly Unusual SiO Maser Source with a Bipolar Nebulosity, IRAS 19312+1950
- Detection of Bipolar Flow toward an Unusual SiO Maser Source IRAS 19312+1950
- Relation of SiO maser emission to IR radiation in evolved stars based on the MSX observation
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- Maser Observations of Westerlund 1 and Comprehensive Considerations on Maser Properties of Red Supergiants Associated with Massive Clusters
- Maser Properties of the Enigmatic IRAS Source 19312+1950
- Quasi-simultaneous 43 and 86 GHz SiO Maser Observations and Potential Bias in the BAaDE Survey Are Resolved
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- Pilot VLBI Survey of SiO v=3 J=1--0 Maser Emission around Evolved Stars
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- Long-term Simultaneous Monitoring Observations of SiO and H2O Masers toward the Mira Variable WX Serpentis