(5 ) C: AAO
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1 C: MPIA
2 (5 ) C: AAO
3 C: AAO
4 C: AAO
5 C: NAOJ C: NAOJ 8.2 m
6 C: Google map C: NAOJ 4200m!
7
8 ( ) ( )
9 1054 ( M1) C: NASA/HST
10
11 C: NASA/Chandra 1006
12 1572 Stella Nova 1604 Astronomie+Populaire ++ by+camille+flammarion+(paris,+1884)
13 1572 ( ) C: NASA/Chandra/MPIA
14 1604 ( ) C: NASA/Chandra
15 1987
16 C: NASA/HST
17 ( ) ( ) SN ? SN ? ? SN SN 1987A
18 100,000 (10 18 km) C: R. Hurt 3 ( km)
19 C: CFHT
20 ( )
21 C: NASA/HST
22 C: Donald P. Waid
23 C: B. J. Fulton
24 C: SDSS
25 C: NASA/Chandra/MPIA km
26 = km 400 = 120,000 = 2,000,000 (2 x 10 6 ) = / (2 x 10 6 ) = 5 x 10 7 km/ ~ 10 4 km/ km
27 km C: NASA
28 C: NASA/Chandra/ MPIA C: NASA/HST 500
29
30 * 10 (C: Essay Web)
31
32
33
34 C: AAO
35 C: NASA/HST Relative flux + const Rest wavelength (Å)
36 C: NASA/HST
37
38
39 (km) Sumiyoshi+05, ApJ, 629, 922 ( )
40 Takiwaki et al D2U
41
42
43
44 C: NAOJ C: NAOJ 8.2 m
45 C: NASA/HST Relative flux + const Rest wavelength (Å)
46 C: NASA/Chandra/ MPIA 1 C: NASA/HST 1
47 a 2 September 2008 Towards remnant 00:52:18 00:52:14 00:52:10 00:52:06 Right ascension Declination a 2 September Declination Towards remnant 00:52:18 00:52:14 00:52:10 00:52:06 Right ascension 0.1
48 a width of 9,000 km s at half maximum. The absorption minimum 21 of the line corresponds to a velocity of 12,000 km s タイムマシン で10,18, typical for normal type Ia supernovae at maximum brightness. Other strong 硫黄 鉄 Ca II OI Si II カルシウム ケイ素 ティコの超新星 銀河系外の超新星 Nugent normal type Ia SN 1994D High-velocity Ca II SN 1572 (Tycho) SN 2001el 00:52:18 00:52:14 00:52:10 00:52:06 Right ascension, Max-Planck-Institut fu r Astronomie, Ko nigstuhl 17, Heid Kashiwa, Chiba , Japan. 3Department of Astronomy, G National Astronomical Observatory of Japan, 650 North A oho The Netherlands. Overluminous type Ia Krause, MT+2008 Nature, 456, Hz 1) 4,000 4,500 5,000 5,500 6,000 6,500 7,000 7,500 8,000 8,500 9,000 Rest wavelength (Å) Towards remnant 1 1 Flux (erg cm 2 s 1 Hz 1) Si II Mg II Si III Fe II Si II Fe III S II S II Na I + Si II ティコの超新星を見てきた supernovae of different lu C: NASA/Chandra/ type Ia supernovae, such as MPIA peculiarities in thei showed lacked a well-defined Si light, although the subseq type Ia supernovae. The lack in the time-averaged spectru in our spectrum of SN 1572 characteristic deep absorp attributed to Ti (ref. 20) not seen for SN The s a 2 September 2008 obtained in the same way available at do not provide a good matc tive values of x and x A well-established corr Dm15(B) of the supernova B remnant has allowed detailed studies, such as tification of the binary companion6, and provid tunity to test theories of the explosion mechanis the progenitor. The determination of the hi spectroscopic type of this supernova is crucia results to the diverse population of type Ia sup II report an optical spectrum of Tycho s superno brightness, obtained from a scattered-light ec centuries after the direct light from the explos Earth. We find that SN 1572 belongs to the majo type Ia supernovae. The supernova of 1572 marked a milestone in th Danish astronomer Tycho Brahe concluded from vations of the new star in the constellation of Ca be located far beyond the Moon11. This co Aristotelian concept, that a change on the sky ca sublunar regime, ultimately led to the abandonm II the immutability of the heavens. The classificat Declination
49 Astronomie+Populaire ++ by+camille+flammarion+(paris,+1884) a 2 September Declination Towards remnant 00:52:18 00:52:14 00:52:10 00:52:06 Right ascension 1572
50 Kepler 0.6 SN kpc Galactic center 0 kpc -5 Tycho sun Crab -10 Cas A kpc C: NASA/Chandra/HST
51 C: NASA/Chandra/ MPIA >1000 C: NASA/HST 1
52 4D2U C: NASA/HST C: NASA (1 30 ) 1 38 km
53 C: NAOJ
54 C: NAOJ
55 4D2U C: NAOJ = 6 10 = 5000
56 C: NAOJ
57 30m -TMT- 30m C: NAOJ
58 すばる望遠鏡で 10年かけて観測した数 TMTでわずか1年 1054年の超新星 かに星雲 の タイムマシン 観測
59 TMT
60
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1 17 object 1 observation 17.1 X electromagnetic wave photon 1 = c (17.1) c =3 10 8 ms ;1 m mm = 10 ;3 m m =10 ;6 m nm = 10 ;9 m 1 Hz 17.1 spectrum radio 2 infrared 3 visual light optical light 4 ultraviolet
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Title 外傷性脊髄損傷患者の泌尿器科学的研究第 3 報 : 上部尿路のレ線学的研究並びに腎機能について Author(s) 伊藤, 順勉 Citation 泌尿器科紀要 (1965), 11(4): 278-291 Issue Date 1965-04 URL http://hdl.handle.net/2433/112732 Right Type Departmental Bulletin Paper
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