不同形狀的行星狀星雲的分布
不同形狀的行星狀星雲的分布
不同形狀的行星狀星雲的分布
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
中 華 民 國 第 四 十 四 屆 中 小 學 科 學 展 覽 會<br />
作 者 說 明 書<br />
高 中 組 地 球 科 學 科<br />
040503<br />
臺 北 市 立 第 一 女 子 高 級 中 學<br />
指 導 老 師 姓 名<br />
吳 育 雅<br />
作 者 姓 名<br />
張 雅 欣<br />
陳 柏 因
44
[He II][a V][O III]<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
2001 <br />
<br />
, <br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
1
1956 Josif S. Shklovsky <br />
<br />
<br />
1966 George Abell Peter Goldreich <br />
<br />
<br />
1967 NGC7027 <br />
<br />
<br />
<br />
<br />
Sun Kwok, Chris R.<br />
Purton M. Pim FitzGerald <br />
<br />
Sun Kwok 1978<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
2
1987 B Balick <br />
<br />
<br />
Manchado2000<br />
<br />
Manchado <br />
1.<br />
-11 <br />
Acker 2 <br />
3.<br />
<br />
H<br />
<br />
<br />
quadrupolar <br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
3
( )<br />
<br />
<br />
Gallery of Planetary Nebula<br />
Spectra <br />
Gallery of Planetary Nebula Spectra <br />
<br />
Flux(ergs/cm 2 /s/a)<br />
<br />
<br />
Gallery of Planetary Nebula Spectra <br />
<br />
<br />
[He II][a V][N II][O III]<br />
<br />
log <br />
<br />
<br />
[He II][a V][O III]<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
http://cf.williams.edu/public/nebulae/browse.cfm<br />
<br />
<br />
Manchado2000 <br />
<br />
<br />
4
HeII <br />
& CA V<br />
He IICa V <br />
( Flux(ergs/cm 2 /s/a))log <br />
<br />
He II Ca V <br />
Log(Flux)<br />
<br />
<br />
Log(Flux)<br />
He II & O III<br />
He IIO III <br />
<br />
Log(Flux)<br />
Log(Flux)<br />
<br />
5
3Ca V& O III<br />
Ca V& O III <br />
Log(Flux)<br />
<br />
Log(Flux)<br />
4He II & N II<br />
He II & N II <br />
<br />
<br />
<br />
Log(Flux)<br />
<br />
Log(Flux)<br />
6
Ca V & N II<br />
<br />
Ca V & N II <br />
<br />
Log(Flux)<br />
<br />
Log(Flux)<br />
O <br />
III & N II<br />
O III & N II <br />
Log(Flux)<br />
<br />
Log(Flux)<br />
<br />
[He II][a V][O III]<br />
[N<br />
II]<br />
<br />
<br />
<br />
[He II][a V][O III]<br />
<br />
<br />
<br />
<br />
39 <br />
27 7
15 12 <br />
<br />
<br />
Ca V <br />
<br />
<br />
<br />
O III <br />
Ca V <br />
8
He II <br />
<br />
<br />
<br />
<br />
~<br />
<br />
<br />
<br />
<br />
<br />
<br />
IC4593NGC6210NGC7009<br />
NGC3242 IC418<br />
FLIERs <br />
FLIERs <br />
<br />
2000/12/15M57 --<br />
<br />
<br />
<br />
<br />
>0 10 ( ) 5 ( )<br />
NGC7662<br />
IC2448<br />
NGC5882<br />
NGC6790<br />
NGC2867<br />
NGC3918<br />
NGC7027<br />
Hb12<br />
NGC2440<br />
NGC7026<br />
<br />
<br />
NGC7009 NGC6210 NGC3242<br />
IC4593<br />
<br />
<br />
IC418<br />
10
NGC2438<br />
NGC6720<br />
NGC6563<br />
NGC6894<br />
NGC40<br />
NGC3195<br />
He2-115<br />
NGC5307<br />
<br />
NGC650<br />
NGC6578<br />
<br />
NGC7293<br />
NGC3587<br />
<br />
<br />
NGC650He2-115 <br />
<br />
<br />
<br />
<br />
<br />
1<br />
2<br />
<br />
11
3<br />
13.58 18.84<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
B.Balick <br />
<br />
<br />
2000<br />
<br />
<br />
<br />
<br />
<br />
(<br />
)<br />
<br />
<br />
De Marco Kitt Peak 3.5 WIYN 11 <br />
<br />
<br />
NoamSoker 1990 <br />
<br />
(Sky & Telescope: November 1997, page 20, and August 2001, page 23)<br />
<br />
<br />
39 <br />
<br />
<br />
<br />
<br />
12
[He II] 5411A(54.4eV)[a V] 6087A67.1 eV [O III] 5007A54.9 eV<br />
<br />
<br />
[He II][a V][O III]<br />
<br />
, <br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
(2002)<br />
<br />
L. Stanghellini, R. L. M. Corradi, and H. E. Schwarz, 1993 ”The correlations between<br />
planetary nebula morphology and central star evolution” Astron. Astrophys. 279,<br />
521-528.<br />
Sun kwok1996,A modern view of planetary nebula, Sky&Telescope, July<br />
1996,p38-43<br />
Sun Kwok1998<br />
Like butterflies from their cocoons, beautiful nebulae emerge from<br />
the dusty shrouds of aging stars , Sky&Telescope, October 1998, p31-36<br />
A. Manchado, E. Villaver, L. Stanghellini, and M. A. Guerrero,2000”The <br />
Morphological and Structural Classification of Planetary Nebulae”,<br />
http://skyandtelescope.com/news/article_1169_1.asp<br />
http://cf.williams.edu/public/nebulae/browse.cfm<br />
http://www.blackskies.com/imageidx.htm <br />
<br />
astro-ph/0002073.<br />
13
[He II] 5411A(54.4eV)[a V] 6087A67.1 eV [O III] 5007A54.9 eV<br />
<br />
<br />
[He II][a V][O III]<br />
<br />
, <br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
(2002)<br />
<br />
L. Stanghellini, R. L. M. Corradi, and H. E. Schwarz, 1993 ”The correlations between<br />
planetary nebula morphology and central star evolution” Astron. Astrophys. 279,<br />
521-528.<br />
Sun kwok1996,A modern view of planetary nebula, Sky&Telescope, July<br />
1996,p38-43<br />
Sun Kwok1998<br />
Like butterflies from their cocoons, beautiful nebulae emerge from<br />
the dusty shrouds of aging stars , Sky&Telescope, October 1998, p31-36<br />
A. Manchado, E. Villaver, L. Stanghellini, and M. A. Guerrero,2000”The <br />
Morphological and Structural Classification of Planetary Nebulae”,<br />
http://skyandtelescope.com/news/article_1169_1.asp<br />
http://cf.williams.edu/public/nebulae/browse.cfm<br />
http://www.blackskies.com/imageidx.htm <br />
<br />
astro-ph/0002073.<br />
13
Change language