dilate 发表于 2025-3-21 19:01:53

书目名称Globular Clusters - Guides to Galaxies影响因子(影响力)<br>        http://figure.impactfactor.cn/if/?ISSN=BK0387017<br><br>        <br><br>书目名称Globular Clusters - Guides to Galaxies影响因子(影响力)学科排名<br>        http://figure.impactfactor.cn/ifr/?ISSN=BK0387017<br><br>        <br><br>书目名称Globular Clusters - Guides to Galaxies网络公开度<br>        http://figure.impactfactor.cn/at/?ISSN=BK0387017<br><br>        <br><br>书目名称Globular Clusters - Guides to Galaxies网络公开度学科排名<br>        http://figure.impactfactor.cn/atr/?ISSN=BK0387017<br><br>        <br><br>书目名称Globular Clusters - Guides to Galaxies被引频次<br>        http://figure.impactfactor.cn/tc/?ISSN=BK0387017<br><br>        <br><br>书目名称Globular Clusters - Guides to Galaxies被引频次学科排名<br>        http://figure.impactfactor.cn/tcr/?ISSN=BK0387017<br><br>        <br><br>书目名称Globular Clusters - Guides to Galaxies年度引用<br>        http://figure.impactfactor.cn/ii/?ISSN=BK0387017<br><br>        <br><br>书目名称Globular Clusters - Guides to Galaxies年度引用学科排名<br>        http://figure.impactfactor.cn/iir/?ISSN=BK0387017<br><br>        <br><br>书目名称Globular Clusters - Guides to Galaxies读者反馈<br>        http://figure.impactfactor.cn/5y/?ISSN=BK0387017<br><br>        <br><br>书目名称Globular Clusters - Guides to Galaxies读者反馈学科排名<br>        http://figure.impactfactor.cn/5yr/?ISSN=BK0387017<br><br>        <br><br>

类型 发表于 2025-3-21 23:55:15

https://doi.org/10.1007/978-3-0348-0018-1a of their integrated light. To do this, we are using a “training set” of spatially resolved clusters. We scan these clusters to obtain integrated light spectra, and also take spectra of individual stars in these clusters to obtain “fiducial” abundances by the usual analysis methods. We briefly desc

QUAIL 发表于 2025-3-22 00:29:01

Sectionally Complemented Latticeservations of GC turnoff stars that these abundance anomalies were already present in the gas from which the observed stars formed. This provides undisputed support to the so-called self-enrichment scenario according to which a large fraction of GC low-mass stars have formed from material processed t

分发 发表于 2025-3-22 07:20:35

Mathematics and Its Applicationsandardized protocols, they can be useful for research through appropriate tools developed either by the host facility or by the science end users. These data holdings also have enormous potential for educational purposes from pre-college through non-majors courses and expert course curricula in univ

airborne 发表于 2025-3-22 10:42:28

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上下连贯 发表于 2025-3-22 14:44:03

Sydney Bulman-Fleming,Kenneth McDowell are naturally reproduced by the presence of super-He-rich populations. However, there are no isochrones and self-consistent HB tracks available in the literature that are based on the up-to-date input physics and wide ranges of He and metal abundances. Here we present new sets of .. isochrones and

上下连贯 发表于 2025-3-22 20:01:26

https://doi.org/10.1007/978-3-211-33614-4 and reliable observational datasets (broadband BVI photometry) available for the cluster, both for variable and nonvariable stars, to infer the most likely masses of individual horizontal branch stars by comparison against theoretical evolutionary tracks, suitably transformed to the observational p

得体 发表于 2025-3-22 22:03:59

https://doi.org/10.1007/978-3-663-20491-6ter Survey (ACSVCS) – to observe 100 early-type members of the Virgo Cluster using the .. The properties of the nuclei from this survey are compared with those of the globular clusters. A similar comparison between the nuclei and the supermassive black holes found in many massive galaxies points to

无畏 发表于 2025-3-23 03:05:40

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代理人 发表于 2025-3-23 06:25:16

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查看完整版本: Titlebook: Globular Clusters - Guides to Galaxies; Proceedings of the J Tom Richtler,Søren Larsen Conference proceedings 2009 Springer-Verlag Berlin H