[TABLE XXXIV]
| H. D. | Star | m | H | Class | Metalic Lines | Line Quality | H wings | Sr+ | Si+ | |
|---|---|---|---|---|---|---|---|---|---|---|
| 120198 | 84 | UMa | 5.53 | 6.4 | x | 9 | 10 | |||
| 108662 | 17 | Com | 5.38 | 2.7 | x | 7 | 8 | |||
| 170397 | Br | 2314 | 5.99 | 2.7 | x | h | 6 | 9 | ||
| 133029 | +47° | 2192 | 6.16 | - | x | h | 5 | 11 | ||
| 140160 | Ser | 5.26 | 3.5 | x | 10 | 5 | ||||
| 94334 | Uma | 4.34 | 3.6 | x | s | 2 | 3 | |||
| 58142 | 21 | Lyn | 4.45 | 2.9 | h | - | 4 | |||
| 192913 | +27° | 3668 | 6.69 | - | h | ? | 7 | |||
| 225132 | 2 | Cet | 4.62 | 1.2 | h | - | 4 | |||
| 41841 | 89 | Lep | 5.50 | 2.2 | - | - | ||||
| 222661 | Aqr | 4.62 | 4.8 | h | - | - | ||||
| 87887 | 15 | Sex | 4.6 | 1.9 | - | 5 | ||||
| 213323 | 38 | Peg | 5.51 | 3.3 | - | - | ||||
| 25642 | Per | 4.33 | 2.2 | - | 4 | |||||
| 114330 | Vir | 4.44 | 3.2 | s | - | 3 | ||||
| 109485 | 23 | Com | 4.78 | 4.1 | s | - | 3 | |||
| 103632 | Cra | 5.16 | 3.8 | x | - | - | ||||
| 110411 | Vir | 4.95 | 5.6 | x | - | - | ||||
| 133962 | k | Boo | 5.59 | 4.6 | x | - | - | |||
| 188260 | 13 | Vul | 4.50 | 2.5 | h | x | - | 4 | ||
| 124224 | 12 | 4.90 | 3.8 | - | 11 | |||||
| 183056 | 4 | Cyg | 5.2 | -0.4 | - | 9 | ||||
| 183986 | +35° | 3658 | 6.04 | - | x | - | 5 | |||
| 196502 | 73 | Dra | 5.18 | 1.2 | x | s | 12 | 10 | ||
| 148367 | Oph | 4.68 | 4.3 | x | s | x | 9 | 8 | ||
| 118022 | 78 | Vir | 4.93 | 3.5 | x | 10 | 9 | |||
| 182564 | Dra | 4.63 | 2.9 | x | 7 | 7 | ||||
| 125337 | Vir | 4.60 | -1.9 | x | h | 7 | 6 | |||
| 214734 | 30 | Cep | 5.21 | 1.6 | x | 3? | 5 | |||
| 7804 | 89 | Psc | 5.28 | 4.2 | x | x | 5 | 7 | ||
| 220825 | Psc | 4.94 | - | x | 6 | 7 | ||||
| 72968 | 3 | Hya | 5.61 | 2.8 | x | 6 | 7 | |||
| 56405 | Paris | 8971 | 5.39 | 4.7 | x | s | s | 3? | 6 | |
| 20677 | 32 | Per | 4.98 | 3.8 | x | x | - | 5 | ||
| 48250 | 12 | Lyn | 4.89 | 1.8 | x | x | - | 5 | ||
| 107612 | - | Com | 6.56 | - | x | 9 | - | |||
| 18519,20 | Ari | 4.6 | 1.1 | s | 3 | 3 | ||||
| 107966 | 13 | Com | 5.10 | 2.7 | - | - | ||||
| 108382 | 16 | Com | 5.04 | 0.6 | - | - | ||||
| 108945 | 21 | Com | 5.39 | 1.9 | x | 11 | 9 | |||
| 108642 | +26° | 2138 | 6.48 | - | x | 8 | 6 | |||
| 89904 | 27 | Lmi | 6.1 | 3.0 | x | h | x | 6 | 9 | |
| 108651 | +26° | 2353 | 6.69 | - | x | h | 7 | 6 | ||
| 170296 | Scu | 4.73 | -0.5 | x | h | x | - | 7 | ||
| 115331 | 196 | Cen | 6.0 | 3.4 | h | 9 | - | |||
| 108486 | +26° | 2352 | 6.57 | - | 7 | - | ||||
| 104321 | Vir | 4.57 | 2.2 | 5 | - | |||||
| 222345 | Aqr | 5.16 | 4.6 | x | - | 9 | ||||
| 14690 | 70 | Cet | 5.62 | 4.3 | x | 7 | ? | |||
| 189849 | 15 | Vul | 4.74 | 3.3 | x | s | x | 9 | 6 | |
| 28546 | 81 | Tau | 5.49 | 5.7 | x | 9 | 9 | |||
| 40536 | 2 | Mon | 5.10 | 4.0 | x | h? | 7 | 7 | ||
| 15089 | Cas | 4.59 | 0.5 | x | 12 | 9 | ||||
| 91312 | Gr | 1658 | 4.85 | 5.6 | x | s | x | 5 | 6 | |
| 159560 | Dra | 4.95 | 6.0 | 8 | - | |||||
| 90277 | 30 | Lmi | 4.85 | 5.0 | x | 9 | 9 | |||
| 57749 | 86 | 5.83 | 2.3 | x | 9 | 6 | ||||
| 92787 | 135 | 5.28 | 7.6 | x | s | 9 | 6 | |||
| 112429 | 8 | Dra | 5.27 | 3.0 | x | 7 | 7 | |||
| 28485 | 80 | Tau | 5.70 | 5.8 | h | 6 | 5 | |||
| 28677 | 85 | Tau | 6.04 | - | - | 7 | - | |||
SUBJECT INDEX
- , Class [166]
- classification [168]
- metallic lines and band absorption [167]
- peculiar [172]
- observational material [208]
- Abnormal abundance, effect on
- spectrum [172]
- Abnormal conditions, effect on
- spectrum [171]
- Absent elements [86]
- Absolute magnitudes for Draper
- classes [197]
- Absorbing efficiencies of atoms [136]
- Absorption coefficient [110]
- Absorption lines [11], [50]
- Abundance of atomic species, [135], [177],
- [183]
- Abundance of atoms, terrestrial [5]
- Aluminum [68], [122]
- Arc spectrum [13]
- [Atomic life] [21], [110]
- life, astrophysical [22], [158]
- nucleus [4]
- number [5]
- states, probabilities of [23]
- weights [5]
- Azimuthal quantum number [8], [204]
- Balmer lines in
- stars [166]
- lines, maximum [166]
- series limit [42]
- Barium [85], [126]
- Blackness of continuous background [49]
- Blending of lines [171]
- Bohr’s Table [9]
- Boundary temperature [27]
- Calcium [70], [122]
- Carbon [59], [121], [207]
- compounds [61]
- spectroscopic and chemical valencies [11]
- Central intensities of spectrum lines [51]
- Central temperature [27]
- Chemical symbols [5]
- Chemical valency [10]
- Chromium [77], [124]
- Chromosphere [35], [47], [159]
- Classification, meaning of [190]
- Classification, principles of [191]
- Cobalt [80]
- Color indices of stars [49]
- Conductivities of flames [112]
- Consistency of temperature scale [130]
- Continuous background of stellar
- spectrum [46], [48]
- Copper [80]
- Critical potential [14]
- Critical potential, astrophysical
- determination [156]
- c-stars [173]
- Definitions, index to [203]
- Density and radius of second type
- stars [36]
- Displacement rule [13], [20]
- Draper classes, homogeneity [193]
- Draper system [191]
- Duration of atomic states [21]
- Earth, composition of crust [185]
- origin of [185]
- total, composition of [187]
- Effective level [28], [136]
- Effective temperature [27]
- Effective temperature, Draper
- classes [197]
- Effect of conditions on spectrum [24]
- Electrons, extra-nuclear [8]
- Electron transfer [11]
- Elements [5]
- Elements, in stellar atmospheres [55]
- Emission lines, production of [11], [53]
- Emission lines, stars showing [53]
- Energy distribution in solar spectrum [49]
- Energy distribution in stellar
- spectrum [49]
- Equivalent outer orbits, electronic [10]
- Even number rule [177]
- Excitation [11]
- Excitation potential [15]
- Flash spectrum [40], [53]
- Formulae in theory of ionization [106]
- Fractional concentration [105]
- Furnace experiments [112]
- Galactic concentrations of Draper
- classes [197]
- Gallium [81]
- Gaseous nebulae, continuous
- spectrum [49]
- Giant and dwarf spectra [195]
- Giant and dwarf temperature
- differences [31]
- Helium [58], [121]
- Hot spark [18]
- Hydrogen, atom [12]
- continuous spectrum [57]
- energy levels [13]
- line intensities [121]
- peculiar behavior [56]
- secondary spectrum [56]
- stellar spectra [55]
- Inner quantum number [204]
- Ionization [11], [15], [97]
- as criterion of pressure [44]
- potential [15]
- " and atomic number [20]
- " astrophysical [156]
- " and temperature of
- maximum [157]
- temperature [30]
- temperature scale [33], [132], [133]
- Ionized atom, lines of [101]
- Intensity of lines [23], [116]
- accuracy [118]
- estimation [117]
- observational material [116]
- Intensity scales [117]
- Interior of star, ionization in [18]
- Iron [79], [125]
- Isotopes [5]
- Law of Mass Action [105], [110]
- Lead [86]
- Level of origin of lines [134]
- Life of atom [21]
- Life of atom, astrophysical [22], [158]
- Limit of Balmer series [42]
- Line intensity, data on [121]
- notes on [127]
- unknown lines [207]
- Lines of unknown origin [55]
- Lithium [59]
- Low temperature conditions, stellar
- atmosphere [94]
- Magnesium [67], [122]
- Magnesium, compounds [67]
- Manganese [78], [124]
- Marginal appearance [105], [135], [179]
- Marginal appearance, observational
- data [181]
- Mass numbers of isotopes [5]
- Maximum of lines [106]
- Meteorites, composition [187]
- Molecule, ionization of [19]
- Molybdenum [84]
- Nickel [80]
- Niobium [84]
- Nitrogen [63], [207]
- Nucleus, atomic [4]
- , Class [162]
- Occurrence of elements in stars [5]
- Optical depth [27], [35]
- Origin of line spectra [11]
- Orion nebula, continuous spectrum [49]
- Oxygen [65], [207]
- Oxygen, compounds [66]
- Palladium [84]
- Partial electron pressure [109]
- Partition function [107]
- Percentage of stars in Draper classes [197]
- Photosphere [35], [47]
- Photoelectric ionization [159]
- Physical constants, astrophysical
- evaluation [155]
- Physical constants, required by
- ionization theory [108]
- Potassium [70]
- Pressure, atmospheres of stars [25], [34]
- from Balmer series limit [44]
- from flash spectrum [40]
- from ionization theory [45]
- from line sharpness [38]
- from line width [39]
- from radiative equilibrium [40]
- shift of lines [26], [38]
- summary [45]
- gradient in outer layers of star [34]
- Quantum number [8]
- Quantum relation [11]
- Radiative equilibrium in outer layers
- of star [40]
- Radium [86]
- Radius and density of second type
- stars [36]
- Rare earths [85]
- Relative abundance of atoms,
- estimation [183]
- abundance of atoms in stellar
- atmosphere [177]
- intensities of spectrum lines [23]
- Reorganization time, see [atomic life]
- Residual intensity [51]
- Reversing layer [50]
- Reversing layer, mass and
- dimensions [47]
- Rhodium [84]
- Rubidium [81]
- Ruthenium [84]
- Rydberg constant [14], [155], [204]
- Saturation [52], [135]
- Scandium [72], [123]
- Series notation [55]
- Silicon [24], [68], [122]
- Silicon stars [169]
- Silver [84]
- Sodium [67]
- Sodium atom [8]
- Solar atmosphere [47]
- energy distribution [49]
- intensities [113]
- Space numbers for Draper classes [197]
- Spark spectrum [14]
- Special problems in stellar
- atmospheres [161]
- [Spectroscopic] valency electrons [10]
- Stark effect [26]
- Stars used for intensity estimates [119]
- Stellar atmosphere compared with
- earth’s crust [184]
- Stellar reversing layer [91]
- Strontium [81], [126]
- Strontium stars [169]
- Structure of absorption line [180]
- Subordinate lines [12]
- Subordinate series [99]
- Sulphur [70], [207]
- Surface gravity [35], [36]
- Symmetry number, see [spectroscopic]
- valency electrons
- Temperature class [24], [112]
- scale [28], [33]
- scale, ionization [33], [133]
- bright stars [31]
- giant and dwarf [31]
- Theory of solution [110]
- Tin [85]
- Titanium [72], [123]
- Titanium compounds [75]
- Total pressure in stellar atmospheres [110]
- Total quantum number [8]
- Typical giant star [41]
- Ultimate lines [11], [94], [111]
- Uniformity of stellar atmospheres [178]
- Valency, chemical [10]
- Valency, spectroscopic [10]
- Vanadium [75], [124]
- Weights of atomic states [107]
- Width of lines [39]
- Wings [51]
- Wolf-Rayet stars [164]
- absorption in [164]
- continuous spectrum [49]
- Yttrium [82], [129]
- Zeemann effect [25]
- Zinc [80], [126]
- Zirconium [83]
NAME INDEX
- Abbot [30], [48], [51]
- Adams [54], [75], [140], [149], [192], [195]
- Anderson [26]
- Aston [5]
- Babcock [23], [38]
- Baillaud [48]
- Baldet [62]
- Baxandall [55], [63], [64], [149], [172], [173]
- Belopolsky [173]
- Bohr [8], [42], [108]
- Bottlinger [51]
- Bowen [18]
- Brandt [17]
- Brill [29]
- Brooks [68]
- Brooksbank [66]
- Burns [159]
- Butler [63]
- Campbell, W. W. [60], [163]
- Cannon, A. J. [54], [163], [190], [198]
- Catalan [17], [77], [84]
- Chenault [17]
- Clarke, F. W. [5], [184], [185], [187]
- Coblentz [30]
- Compton, K. T. [17], [56], [59]
- Cortie [66]
- Coster [23]
- Curtis [159]
- Curtiss [58]
- Davies [17], [19]
- de Forcrand [60]
- de Gramont [59], [111]
- Dempster [22]
- Deslandres [58]
- Dorgelo [23]
- Duffendack [19]
- Dyson [86]
- Eddington [27], [34], [41], [53], [180]
- Einstein [23], [113], [163]
- Eldridge [17]
- Evershed [26], [38], [58], [62]
- Fairfield [56], [57], [159]
- Fermi [23]
- Foote [17]
- Fowler, A., [11], [14], [17], [38], [56], [60],
- [62], [65], [66], [68], [75], [186], [191]
- Fowler, R. H., [17], [37], [44], [61], [70],
- [93], [106-110], [108], [133], [135], [156], [166], [179]
- Franck [19], [22], [43]
- Füchtbauer [23]
- Gale [75]
- Giebeler [86]
- Gieseler [17]
- Gousmid [86]
- Grotrian [17], [22]
- Guckel [60]
- Hale [25], [75]
- Harper [79], [117], [176], [192]
- Harrison [181]
- Hartley [81]
- Hartmann [71]
- Hartree [17], [61]
- Heger [67], [72]
- Hertzsprung [31], [175]
- Hoffmann [23]
- Hopfield [17], [186]
- Horton [17], [19]
- Howe [43]
- Hubble [49], [57]
- Huggins [57]
- Hulburt [26]
- Huthsteiner [17]
- Jeffreys [185]
- Johnson, M. C. [53], [85]
- Johnson, R. C. [62]
- Joy [54], [149], [192], [195]
- Kiess, C. C. [13], [17], [72], [84], [86], [173]
- Kiess, H. K. [17]
- King, A. S. [24], [38], [69], [84], [112]
- King, E. S. [29]
- Knipping [19]
- Kohlschütter [51], [140]
- Kohn [60]
- Kossell [13], [21]
- Kramers [8], [23]
- Krüger [19]
- Landé [25]
- Lee [71]
- Lindblad [48], [57], [62], [169]
- Lindemann [26]
- Lockyer, J. N. [64], [70], [172], [173]
- Lundmark [198]
- Lunt [6], [85]
- Luyten [67], [162], [170]
- Lyman [18], [57], [58]
- Maury [173]
- McLennan [18], [63]
- Meggers [13], [17], [72], [75], [82]
- Menzel [44], [66-68], [71], [74-76], [79-81], [85],
- [109], [116], [133], [166], [181]
- Merrill, G. P. [817]
- Merrill, P. W. [54], [83]
- Merton [25], [60], [62]
- Mie [22]
- Millikan [18]
- Milne [17], [22], [28], [36], [37], [44], [48], [50], [61],
- [70], [93], [97], [106-110], [113], [133], [135], [140],
- [156], [158], [166], [179]
- Mitchell [58], [86]
- Mohler [17]
- Mulliken [61]
- Newall [63]
- Nicholson, J. W. [43]
- Noyes [112]
- Pannekoek [35], [140]
- Paschen [14], [17], [156]
- Payne [20], [38], [43], [58], [60], [68], [156],
- [163], [183]
- Plaskett, H. H. [14], [30], [48], [51], [54], [59],
- [60], [64], [65], [85], [156], [163], [184]
- Plaskett, J. S. [60], [71], [162], [163], [171]
- Pluvinel [62]
- Ramage [81]
- Rognley [17]
- Rosenberg [29]
- Rowland [127]
- Ruark [17]
- Rufus [62], [72]
- Russell [17], [26], [37], [39], [40], [44], [47],
- [52], [55], [56], [59], [70], [79], [80], [110], [175], [178],
- [184], [203]
- Saha [43], [85], [105], [113]
- St. John [25], [38]
- Sampson [30]
- Saunders [38], [55], [203]
- Scheiner [29]
- Schwarzschild [51], [137], [160]
- Seares [31]
- Shane [62]
- Shapley [36], [40], [51], [62], [162], [168],
- [170], [185], [198]
- Shaver [17]
- Shrum [64]
- Slipher [75]
- Smyth [17], [19]
- Sommerfeld [13], [17], [21], [23]
- Sponer [17]
- Stark [25]
- Stewart [26], [37], [39], [40], [44], [47], [91], [110], [175]
- Strutt [66]
- Takamine [26]
- Tate [17]
- Thomas [18]
- Turner [22]
- Udden [17]
- Urey [108]
- Van Maanen [162]
- Vegard [63]
- Violle [60]
- Von Zeipel [185]
- Walters [13], [72], [77], [79]
- Washington [5], [184], [185]
- Webb [22]
- Wien [22]
- Wilsing [29], [48]
- Wilson, E. B. [162]
- Wilson, H. A. [112]
- Wilson, H. H. [162]
- Woltjer [113]
- Wood [22], [42], [57]
- Wright [43], [56], [57], [66], [163], [173]
- Young [79], [117], [176], [192]
- Zeemann [25]