A・一般) ＣＣＳゼーマン効果と理論計算を連携させた星形成における磁場の
A・一般) ＣＣＳゼーマン効果と理論計算を連携させた星形成における磁場の
A・一般) ＣＣＳゼーマン効果と理論計算を連携させた星形成における磁場の
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Target Core Pilot Survey<br />
<br />
<br />
<br />
To successfully detect the Zeeman splitting, sample<br />
selection is extremely important.<br />
strong CCS emission + narrow line widths<br />
pilot observations<br />
OTF observations with S40+AC<br />
Hirota et al. (2009,2011)<br />
position switch observations<br />
observations done by Tanaka<br />
41 0<br />
K km/s<br />
0.7<br />
0.6<br />
L1495B<br />
T peak ~ 2.5 K<br />
V ~ 0.25 km/s<br />
0.5<br />
DEC (1950)<br />
40 0<br />
39 0<br />
0.4<br />
0.3<br />
0.2<br />
T A<br />
*<br />
(K)<br />
28 38 0<br />
0.1<br />
12m40s 12m35s 12m30s 4h12m25s<br />
RA (1950)<br />
0.0<br />
V LSR (km/s)<br />
9
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