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標(biāo)題: Titlebook: Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries; S. Flügge Book 1958 Springer-Verlag OHG. Berlin [打印本頁]

作者: 和尚吃肉片    時間: 2025-3-21 17:23
書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries影響因子(影響力)




書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries影響因子(影響力)學(xué)科排名




書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries網(wǎng)絡(luò)公開度




書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries被引頻次




書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries被引頻次學(xué)科排名




書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries年度引用




書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries年度引用學(xué)科排名




書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries讀者反饋




書目名稱Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries讀者反饋學(xué)科排名





作者: 實現(xiàn)    時間: 2025-3-21 21:12
Loading Methods Specific to Flex,ierung der Nebelphysik zu entwickeln. Letzteres geschieht gesondert in dem zweiten Artikel am Ende dieses Bandes (S. 399). Beide Artikel sind als zusammengeh?rig und als sich gegenseitig erg?nzend zu betrachten.
作者: 離開就切除    時間: 2025-3-22 03:12

作者: 自負(fù)的人    時間: 2025-3-22 06:50
Foundation XML and E4X for Flash and Flexies of binaries may generally be safely ignored.. The former case of the true ., or ., is the topic of the present article. While no fundamental distinction may exist between binaries, multiple stars, associations, and star clusters, the designation “visual binary” refers to pairs of stars falling within arbitrary, limited angular separations.
作者: 柔美流暢    時間: 2025-3-22 11:10
Visual Binaries,ies of binaries may generally be safely ignored.. The former case of the true ., or ., is the topic of the present article. While no fundamental distinction may exist between binaries, multiple stars, associations, and star clusters, the designation “visual binary” refers to pairs of stars falling within arbitrary, limited angular separations.
作者: Chronic    時間: 2025-3-22 14:53

作者: 證實    時間: 2025-3-22 19:10

作者: 男學(xué)院    時間: 2025-3-23 01:15

作者: 夸張    時間: 2025-3-23 04:12
Die Spektren der planetarischen Nebel,ierung der Nebelphysik zu entwickeln. Letzteres geschieht gesondert in dem zweiten Artikel am Ende dieses Bandes (S. 399). Beide Artikel sind als zusammengeh?rig und als sich gegenseitig erg?nzend zu betrachten.
作者: CLAY    時間: 2025-3-23 06:44

作者: Allodynia    時間: 2025-3-23 11:28

作者: Arboreal    時間: 2025-3-23 17:19

作者: hallow    時間: 2025-3-23 20:51

作者: 平躺    時間: 2025-3-24 01:11

作者: dura-mater    時間: 2025-3-24 06:05
https://doi.org/10.1007/978-1-4302-1635-3Une monographic complète sur I’astrophysique moléculaire exigerait, ? eile seule, un gros volume. Notre but a été modeste: nous avons simplement tenté de décrire les principales observations et d’esquisser les idées générales essentielles concernant le r?le joué par les molécules dans les atmosphères stellaires.
作者: 表示向下    時間: 2025-3-24 08:34

作者: 標(biāo)準(zhǔn)    時間: 2025-3-24 13:34

作者: cataract    時間: 2025-3-24 15:57

作者: larder    時間: 2025-3-24 21:53
,Les bandes moléculaires dans les spectres stellaires,Une monographic complète sur I’astrophysique moléculaire exigerait, ? eile seule, un gros volume. Notre but a été modeste: nous avons simplement tenté de décrire les principales observations et d’esquisser les idées générales essentielles concernant le r?le joué par les molécules dans les atmosphères stellaires.
作者: Infantry    時間: 2025-3-25 01:37

作者: 松果    時間: 2025-3-25 04:43

作者: dragon    時間: 2025-3-25 09:40

作者: Intentional    時間: 2025-3-25 13:10

作者: thrombus    時間: 2025-3-25 17:18

作者: Hippocampus    時間: 2025-3-25 21:02

作者: Living-Will    時間: 2025-3-26 03:34
https://doi.org/10.1007/978-1-4302-1635-3 spectral lines. If, in the spectrum of a star, two sets of spectral lines can be observed which oscillate in opposite directions, the star is called a double- lined spectroscopic binary. If only one set of lines is present, the star is called a single-lined spectroscopic binary. Many intrinsic vari
作者: voluble    時間: 2025-3-26 05:09

作者: 令人悲傷    時間: 2025-3-26 09:28
Astrophysik I: Sternoberfl?chen-Doppelsterne / Astrophysics I: Stellar-Surfaces-Binaries978-3-642-45906-1Series ISSN 0085-140X Series E-ISSN 2197-4195
作者: enchant    時間: 2025-3-26 15:25

作者: 憂傷    時間: 2025-3-26 17:36

作者: CRAMP    時間: 2025-3-26 22:05
The Spectra of the White Dwarfs,nd spectra. Theoretical development in model stellar atmospheres, in the theory of line broadening, and more data on parallaxes are badly needed. Nevertheless we now approach a period in which interpretation of white-dwarf spectra in terms of composition will become profitable.
作者: 考博    時間: 2025-3-27 01:50

作者: 歸功于    時間: 2025-3-27 08:48
Stars with Peculiar Spectra,r spectra into some sort of sequence, those which fit into the sequence (i.e., classification) defined by the majority automatically become “normal”, while those which cannot be dropped into any of the normal classes are naturally called “pecuhar”. Some extreme cases will always be listed as peculia
作者: 西瓜    時間: 2025-3-27 11:42

作者: 的染料    時間: 2025-3-27 15:56
The Spectra of the White Dwarfs,of astrophysics [.]. After an early period of observation, an extremely successful and complete theory of their structure was developed [.]. These stars are faint both intrinsically and by apparent magnitude, and detailed investigation of their spectra, colors, parallaxes and masses have been few an
作者: Epithelium    時間: 2025-3-27 21:34
Visual Binaries,e direction, but at widely differing distances. The latter case represents the so-called ., which is of little or no interest, and in statistical studies of binaries may generally be safely ignored.. The former case of the true ., or ., is the topic of the present article. While no fundamental disti
作者: 場所    時間: 2025-3-27 23:07

作者: Serenity    時間: 2025-3-28 04:47

作者: 迷住    時間: 2025-3-28 08:45
Klaus Regenauer-Lieb,David A. Yuen,Florian Fusseisr erziehungswissenschaftlichen Diskussion Auftrieb verschafften:.Um gr??ere Klarheit zu erlangen, scheint es sinnvoll, zun?chst vom Begriff des Lernens auszugehen, um erst dann zu ergründen, was “Offenheit” in bezug auf Lernen meinen kann. Bei meinem Verst?ndnis von Lernen beziehe ich mich auf Günth
作者: arbiter    時間: 2025-3-28 13:09
Peter Armstrongcal representation of general recoupling coefficients, and the studies on the tree cover number are motivated by its equality with the maximum positive semidefinite nullity on multigraphs with treewidth at most two..Given the interest in the tree cover number on graphs with bounded treewidth, we inv
作者: entreat    時間: 2025-3-28 16:42
Vulnerabilities in Local Contexts decrease the probability of unemployment exits in deprived neighbourhoods; (3) that people residing in locations with higher levels of income inequality perceive others as being more competitive, which produces paradoxical effects on their self-rated health and undermines the psychological health o
作者: curettage    時間: 2025-3-28 21:00
Pieter De Koninck,Jochen De Weerdtrd relaying scheme is considered, which decodes the received data and then retransmits the re-encoded data and removes the noise present. The expressions are derived for probability density function (PDF), cumulative distributive function (CDF), and outage probability in terms of Meijer G-function.
作者: 盲信者    時間: 2025-3-29 02:21

作者: 鉤針織物    時間: 2025-3-29 05:56
Addendumroup and 5 of the non-cancerous group. In the other 18 clusters the other non-cancerous patients were grouped. In this way, out of 42 cancerous patients 34 had been grouped into C. or C. and out of 348 non-cancerous patients 339 were grouped into the 18 clusters except for 9 patients who appeared in




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