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molecules:ism:sio [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:sio [2019/10/18 12:56] (current) – mueller | ||
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R. W. Wilson, A. A. Penzias, K. B. Jefferts, M. Kutner, and P. Thaddeus\\ | R. W. Wilson, A. A. Penzias, K. B. Jefferts, M. Kutner, and P. Thaddeus\\ | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
The //J// = 3 – 2 transition of SiO near 130.2 GHz was detected in emission with the 11 m Kitt Peak telescope toward Sgr B2(OH).\\ | The //J// = 3 – 2 transition of SiO near 130.2 GHz was detected in emission with the 11 m Kitt Peak telescope toward Sgr B2(OH).\\ | ||
D. F. Dickinson\\ | D. F. Dickinson\\ | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
The 11 m Kitt Peak telescope was used to detect the line toward Sgr B2(OH) and Orion A. | The 11 m Kitt Peak telescope was used to detect the line toward Sgr B2(OH) and Orion A. | ||
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P. Schilke, G. Pineau des Forêts, C. M. Walmsley, and J. Martín-Pintado\\ | P. Schilke, G. Pineau des Forêts, C. M. Walmsley, and J. Martín-Pintado\\ | ||
performed\\ | performed\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
The IRAM 30 m telecope was used to detect several SiO transitions toward the Orion Bar and S 140. | The IRAM 30 m telecope was used to detect several SiO transitions toward the Orion Bar and S 140. | ||
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S. Yamamoto, H. Mikami, S. Saito, N. Kaifu, M. Ohishi, and K. Kawaguchi\\ | S. Yamamoto, H. Mikami, S. Saito, N. Kaifu, M. Ohishi, and K. Kawaguchi\\ | ||
detected\\ | detected\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
//Publs. Astron. Soc. Japan// **167**, L97–L100 (1971),\\ | //Publs. Astron. Soc. Japan// **167**, L97–L100 (1971),\\ | ||
a low-mass star-forming region. | a low-mass star-forming region. | ||
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The molecule is conspicuously absent in cold, quiescent molecular clouds, as reported by\\ | The molecule is conspicuously absent in cold, quiescent molecular clouds, as reported by\\ | ||
L. M. Ziurys, P. Friberg, and W. M. Irvine,\\ | L. M. Ziurys, P. Friberg, and W. M. Irvine,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
The absence of SiO was reported for TMC-1, L134N (aka L183) and for B335 (aka L663). Hence,\\ | The absence of SiO was reported for TMC-1, L134N (aka L183) and for B335 (aka L663). Hence,\\ | ||
J. Martin-Pintado, | J. Martin-Pintado, | ||
view\\ | view\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
L. E. Snyder and D. Buhl\\ | L. E. Snyder and D. Buhl\\ | ||
proposed the\\ | proposed the\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
Orion A was observed with the 11 m Kitt Peak telescope. The frequency coincidence with the //J// = 2 – 1 transition of SiO in its first excited vibrational state was noted.\\ | Orion A was observed with the 11 m Kitt Peak telescope. The frequency coincidence with the //J// = 2 – 1 transition of SiO in its first excited vibrational state was noted.\\ | ||
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J. H. Davis, G. N. Blair, H. van Till, and P. Thaddeus,\\ | J. H. Davis, G. N. Blair, H. van Till, and P. Thaddeus,\\ | ||
who studied\\ | who studied\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
They observed the //J// = 3 – 2 transition of SiO. | They observed the //J// = 3 – 2 transition of SiO. | ||
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D. Buhl, L. E. Snyder, F. J. Lovas, and D. R. Johnson\\ | D. Buhl, L. E. Snyder, F. J. Lovas, and D. R. Johnson\\ | ||
reported subsequently on\\ | reported subsequently on\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
Half of the authors are laboratory spectroscopists, | Half of the authors are laboratory spectroscopists, | ||
Line 55: | Line 55: | ||
T. Kaminski, C. A. Gottlieb, K. H. Young, K. M. Menten, and N. A. Patel\\ | T. Kaminski, C. A. Gottlieb, K. H. Young, K. M. Menten, and N. A. Patel\\ | ||
performed\\ | performed\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
and detected a //v// = 5 SiO maser. | and detected a //v// = 5 SiO maser. | ||
Line 61: | Line 61: | ||
E. Gonzalez-Alfonso, | E. Gonzalez-Alfonso, | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
S.-H. Cho, H.-G. Kim, Y.-S. Park, C.-H. Choi, and N. Ukita\\ | S.-H. Cho, H.-G. Kim, Y.-S. Park, C.-H. Choi, and N. Ukita\\ | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
L. Decin, J. Cernicharo, M. J. Barlow, et al.\\ | L. Decin, J. Cernicharo, M. J. Barlow, et al.\\ | ||
investigated\\ | investigated\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
Using the PACS low-resolution spectrometer on board of the // | Using the PACS low-resolution spectrometer on board of the // | ||
Line 78: | Line 78: | ||
L. Velilla Prieto, C. Sánchez Contreras, J. Cernicharo, M. Agúndez, G. Quintana-Lacaci, | L. Velilla Prieto, C. Sánchez Contreras, J. Cernicharo, M. Agúndez, G. Quintana-Lacaci, | ||
in the course of\\ | in the course of\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
L. Decin, A. M. S. Richards, T. Danilovich, W. Homan, and J. A. Nuth\\ | L. Decin, A. M. S. Richards, T. Danilovich, W. Homan, and J. A. Nuth\\ | ||
reported on an\\ | reported on an\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
The low mass-loss star was R Dor, the high mass-loss star was IK Tau. The very sensitive data permitted detection of < | The low mass-loss star was R Dor, the high mass-loss star was IK Tau. The very sensitive data permitted detection of < |