標(biāo)題: Titlebook: Cool Stars with Excesses of Heavy Elements; Proceedings of the S Mercedes Jaschek,Philip C. Keenan Conference proceedings 1985 D. Reidel Pu [打印本頁] 作者: hormone-therapy 時間: 2025-3-21 16:34
書目名稱Cool Stars with Excesses of Heavy Elements影響因子(影響力)
書目名稱Cool Stars with Excesses of Heavy Elements影響因子(影響力)學(xué)科排名
書目名稱Cool Stars with Excesses of Heavy Elements網(wǎng)絡(luò)公開度
書目名稱Cool Stars with Excesses of Heavy Elements網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Cool Stars with Excesses of Heavy Elements被引頻次
書目名稱Cool Stars with Excesses of Heavy Elements被引頻次學(xué)科排名
書目名稱Cool Stars with Excesses of Heavy Elements年度引用
書目名稱Cool Stars with Excesses of Heavy Elements年度引用學(xué)科排名
書目名稱Cool Stars with Excesses of Heavy Elements讀者反饋
書目名稱Cool Stars with Excesses of Heavy Elements讀者反饋學(xué)科排名
作者: Pedagogy 時間: 2025-3-21 22:10
Reliability Improvement Warranties,e spectra we examine the more evident it becomes that the groups that we are talking about here are practically never discrete and clearly bounded. There always seem to be marginal stars that blur the distinctions between the so-called groups.作者: 無效 時間: 2025-3-22 01:08
The Role of Warranty in Marketing, of CS as well as C stars, though not of SC or S stars and is therefore a sensitive indicator of C/O variation when C/O ? 1.0. The depths of the various absorption features within the spectra of CS stars differ considerably from one star to the next while the SC stars all show very similar spectra. 作者: 正式通知 時間: 2025-3-22 05:40 作者: VOC 時間: 2025-3-22 10:14 作者: 貪婪的人 時間: 2025-3-22 14:07 作者: 貪婪的人 時間: 2025-3-22 17:54
Reliability Improvement Warranties,ristics of H.D. barium-star suspects south of δ = -26? found on moderate-dispersion objective-prism plates. For stars of the type that can be found from such plates, the frequency appears to lie between one-half and one percent.作者: Redundant 時間: 2025-3-22 23:18
Warranty Management and Product Manufactureesponding fluxes and an ultraviolet classification. The preparation of this publication has confirmed that MK classification cannot simply be transferred to the Ultraviolet range..Work on a second part concentrating on peculiar stars is at an advanced stage. More than 650 stars are presently candida作者: Obstruction 時間: 2025-3-23 05:18
Warranty Management and Product Manufactureg II lines are much weaker and low-excitation lines from neutral metals are stronger. Spectra of early R stars (R0–R3) closely resemble those of late G or early K in both lines and continuum with no significant emission lines. Late R stars (R5–R8) show spectra like late K or early M stars except tha作者: Certainty 時間: 2025-3-23 08:02
The Role of Warranty in Marketing,ergy distributions, leading to estimates of effective temperature, tests of model atmospheres, and the detection of companions or circumstellar shells; (3) spectroscopic data from narrow-band photometry of strong spectral features; and (4) light curves of variable stars. The photometric properties o作者: confederacy 時間: 2025-3-23 10:54 作者: 會犯錯誤 時間: 2025-3-23 17:50
Reliability Improvement Warranties,he atmospheric structure of carbon stars: Because of the increased line-blanketing(backwarming) effect due to increased molecular absorption in cooler stars, kinetic temperature of the line formation layers shows little decrease for large decrease of the effective temperature (e.g., △T.(FeI)=250K fo作者: Flustered 時間: 2025-3-23 19:43
Systems Approach to Warranty Management, CN and CH anomalies, metal deficiencies and interstellar reddening. It also turns out to be a very powerful tool for monitoring the variability of the cool stars. The identification of the observed spectra and the computation of the partial pressure versus optical depth via model atmospheres demons作者: OGLE 時間: 2025-3-24 01:27 作者: glowing 時間: 2025-3-24 02:26 作者: esoteric 時間: 2025-3-24 07:16
Identification of Photographic Infrared Spectral Region in Carbon Starsconnection with the identification of .CN, .CN, HCN, [CI] λ8727, and telluric H.O lines. The microphotometric tracing of the same region of an M-type star μ Cep seems very helpful for the identification of telluric H.O lines.作者: 休閑 時間: 2025-3-24 12:13
The Discovery and Frequency of Barium Starsristics of H.D. barium-star suspects south of δ = -26? found on moderate-dispersion objective-prism plates. For stars of the type that can be found from such plates, the frequency appears to lie between one-half and one percent.作者: precede 時間: 2025-3-24 18:19
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/c/image/237886.jpg作者: anticipate 時間: 2025-3-24 22:17
Prevention of Controller Windup,Some correlations between period of pulsation, spectral type at maximum, mean difference in visual magnitude between maxima and minima, intensity of Tc I line, ratio of the number of days from minimum to the next following maximum to the period, and infrared colour index [11μ] ? [3.5 μ] are described for S Mira variables.作者: Hyperopia 時間: 2025-3-25 02:51
Warranty Management and Product ManufactureFor the present conference, the principal interest in studying the distributions and motions of peculiar red giants (in our own and other galaxies) is in the information that this gives us on the population types (ages, masses) and evolutionary phases of these stars.作者: 惡意 時間: 2025-3-25 05:44 作者: 調(diào)色板 時間: 2025-3-25 07:42 作者: cardiovascular 時間: 2025-3-25 11:56
Cool Stars with Excesses of Heavy Elements978-94-009-5325-3Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: extrovert 時間: 2025-3-25 18:00 作者: 使成波狀 時間: 2025-3-25 23:16
Reliability Improvement Warranties,e spectra we examine the more evident it becomes that the groups that we are talking about here are practically never discrete and clearly bounded. There always seem to be marginal stars that blur the distinctions between the so-called groups.作者: 友好 時間: 2025-3-26 02:12
Springer Series in Reliability Engineeringconnection with the identification of .CN, .CN, HCN, [CI] λ8727, and telluric H.O lines. The microphotometric tracing of the same region of an M-type star μ Cep seems very helpful for the identification of telluric H.O lines.作者: acrimony 時間: 2025-3-26 06:27
Reliability Improvement Warranties,ristics of H.D. barium-star suspects south of δ = -26? found on moderate-dispersion objective-prism plates. For stars of the type that can be found from such plates, the frequency appears to lie between one-half and one percent.作者: Suggestions 時間: 2025-3-26 10:10
https://doi.org/10.1007/978-94-009-5325-3Galaxy; LOPES; Libration; earth; galaxies; observatory; photometry; planet; star; stars; stellar; stellar evolu作者: 雜役 時間: 2025-3-26 14:43 作者: 同謀 時間: 2025-3-26 17:34 作者: BROOK 時間: 2025-3-26 21:48 作者: 破裂 時間: 2025-3-27 03:42 作者: bioavailability 時間: 2025-3-27 08:44 作者: enterprise 時間: 2025-3-27 09:42 作者: 支形吊燈 時間: 2025-3-27 16:42
The Catalogue of Stellar Groups. II. Cool Peculiar Starsrresponding volume is expected to be published soon. Histograms in visual magnitudes and plots of the galactic distribution are presented here for some of the groups under discussion during the colloquium.作者: 地殼 時間: 2025-3-27 21:29
The Role of Warranty in Marketing, most 5% of this 1%-. The spectra of these stars are so complex that many astronomers have shied away from studying them. This can be clearly seen in the IAU symposia: of the 111 held to date, none was dedicated to late-type giants, whereas at least four were dedicated to early-type stars.作者: gospel 時間: 2025-3-28 00:48 作者: Platelet 時間: 2025-3-28 04:47
The Role of Warranty in Marketing,sured with theoretical energy distributions. Quantitative classification criteria are derived from measured line and band strengths. At the resolution of our measurements, mildly peculiar stars cannot be easily distinguished from normal stars.作者: STEER 時間: 2025-3-28 07:34 作者: Lipoma 時間: 2025-3-28 11:06 作者: 宏偉 時間: 2025-3-28 16:57
Absolute Spectrophotometry of F-, G-, K-, and M-Type Starssured with theoretical energy distributions. Quantitative classification criteria are derived from measured line and band strengths. At the resolution of our measurements, mildly peculiar stars cannot be easily distinguished from normal stars.作者: 致詞 時間: 2025-3-28 22:33 作者: CARE 時間: 2025-3-28 23:19
Systems Approach to Warranty Management,of different atmospheric layers, and a new photometric system for the monitoring of carbon stars (miras, SRabc, Lbc, RCB, HdC, CH, strong-CN,…) is proposed. The flux variations recorded by well-suited filters are the ground-based material for hydrodynamical investigations of these stars.作者: GUILT 時間: 2025-3-29 07:00 作者: 好色 時間: 2025-3-29 10:03 作者: NEX 時間: 2025-3-29 13:11 作者: Lyme-disease 時間: 2025-3-29 16:23
D.N. Prabhakar Murthy,Wallace R. Blischkeand the “Catalogue of Central Stars of Planetary Nebulae” (Acker, Gleizes et al, 1982), the caracteristics of these peculiar stars have been compared. The intensive spectrographic study undertaken by F. Gleizes (1984) for about 40 nuclei has also been used.作者: ARK 時間: 2025-3-29 21:21
Warranty Management and Product Manufacturered to the Ultraviolet range..Work on a second part concentrating on peculiar stars is at an advanced stage. More than 650 stars are presently candidates for this volume, and the relative frequency of the individual spectral groups is given in Table I with reference to the Catalogue of Stellar Groups.作者: Conserve 時間: 2025-3-30 02:27
Warranty Management and Product ManufactureG or early K in both lines and continuum with no significant emission lines. Late R stars (R5–R8) show spectra like late K or early M stars except that lines from low levels of excitation are stronger. Ultraviolet spectra of S stars show a wide variation in the strength of Mg II lines.作者: Minatory 時間: 2025-3-30 06:27 作者: arbiter 時間: 2025-3-30 10:39
Design of Observer-based Controllers,rresponding volume is expected to be published soon. Histograms in visual magnitudes and plots of the galactic distribution are presented here for some of the groups under discussion during the colloquium.作者: 盡責(zé) 時間: 2025-3-30 12:55 作者: interlude 時間: 2025-3-30 20:32
Spectral Classification and the Relations Between Peculiar Giantse spectra we examine the more evident it becomes that the groups that we are talking about here are practically never discrete and clearly bounded. There always seem to be marginal stars that blur the distinctions between the so-called groups.作者: JOG 時間: 2025-3-30 23:38 作者: 閑逛 時間: 2025-3-31 04:46
Spectrophotometry Characteristics of Barium StarsThese stars with enhanced Ba II at 4554A are otherwise generality similar to late-type giant stars. The majority of them were identified in an objective-prism survey by MacConnell et al. (1972). They listed 150 “certain” and 90 “marginal” Ba stars but made no further estimates of barium intensity. A
