Page 11 - spectroscopic-atlas-5_0-english_Neat

Spectroscopic Atlas for Amateur Astronomers 11

Table Page Topic Objects Wavelength Gra-
domain ting
21 68 Detailed spectrum of an early A- Sirius A α CMa
class star 3900 – 6700 200L
22 3900 – 4700 900L
23 4780 – 5400 900L
30
31 70 Effects of the luminosity on spectra Vega α Lyr 3900 – 4700 900L
40 of the early A-class Ruchbah δ Cas
41 Deneb α Cyg
42
50 71 Metallicity: Vega vs. Sirius Vega α Lyr 3920 – 4700 900L
51 Sirius A α CMa 3830 – 6700 200L
52
53 74 Development of spectral features Adhafera ζ Leo
56 within the F-class Procyon α CMi
59
61 76 Effects of the luminosity on spectra Porrima γ Vir 3920 – 4750 900L
62 of the early F-class Caph β Cas
63 Mirfak α Per
64
64A 79 Development of spectral Muphrid η Boo 3800 – 6600 200L
64B features within the G-class Vindemiatrix ε Vir

80 Detailed spectrum of an early G- Sun 3800 – 7200 200L
class star 3900 – 4800 900L

81 Detailed spectrum of an early G- Sun 4700 – 5700 900L
class star 5650 – 6700

85 Development of spectral features Arcturus α Boo 3900 – 6800 200L
within the K-class Alterf λ Leo

86 Detailed spectrum of an early Pollux α Gem 3900 – 6800 200L
K-class star 3800 – 4800 900L

88 Effects of the luminosity on spectra Alsciaukat α Lyncis 4000 – 4900 900L

of the late K-class 61 Cygni B

89 Detailed spectrum of a later Aldebaran α Tau 5150 – 5900 900L
K-class star 5850 – 6700

92 Development of spectral features Antares α Sco 3900 – 7200 200L
within the M-class Ras Algethi α Her

96 Mira Variable M(e), comparison to Mira o Ceti 3900 – 7200 200L

a late classified M-Star Ras Algethi α Her

99 Extreme S-Class star, comparison R Cygni 4100 – 7300 200L
to a Mira Variable M(e) Mira o Ceti

101 Development of spectral features Omikron1 Orionis 4100 – 7300 200L
within the S-Class Chi Cygni
R Cygni

102 Comparison of an „intrinsic“ and BD Camelopardalis 4300 – 7200 200L
„extrinsic“ S-Class star HR Pegasi

107 Comparison of differently classi- WZ Cassiopeiae 4600 – 7300 200L
fied carbon stars Z Piscium
W Orionis

108 Merrill Sanford Bands, details at a W Orionis 4730 – 5400 900L
higher resolved spectrum 5100 - 7300 200L

109 Carbon star with Hα- emission- R Leporis
line