PED
发表于 2025-3-21 17:52:26
书目名称New Light on Galaxy Evolution影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0665432<br><br> <br><br>书目名称New Light on Galaxy Evolution影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0665432<br><br> <br><br>书目名称New Light on Galaxy Evolution网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0665432<br><br> <br><br>书目名称New Light on Galaxy Evolution网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0665432<br><br> <br><br>书目名称New Light on Galaxy Evolution被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0665432<br><br> <br><br>书目名称New Light on Galaxy Evolution被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0665432<br><br> <br><br>书目名称New Light on Galaxy Evolution年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0665432<br><br> <br><br>书目名称New Light on Galaxy Evolution年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0665432<br><br> <br><br>书目名称New Light on Galaxy Evolution读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0665432<br><br> <br><br>书目名称New Light on Galaxy Evolution读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0665432<br><br> <br><br>
中世纪
发表于 2025-3-21 22:20:50
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补充
发表于 2025-3-22 03:31:08
The Rate of Supernovae in Normal Galaxieslaxy is known. Constraints to the models are the present chemical content of galaxies but also the present observed SN rate (Arimoto & Yoshi, 1987; Ferrini & Poggianti, 1993; Matteucci, 1994; Renzini ..., 1993; Bressan ..., 1994; Elbaz .., 1995).
同谋
发表于 2025-3-22 08:06:30
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Interstellar
发表于 2025-3-22 11:13:50
1743-9213 de variety of recent developments,present new insights and demonstrate the rapid increase in ourknowledge about galaxy evolution and formation.978-0-7923-3976-2978-94-009-0229-9Series ISSN 1743-9213 Series E-ISSN 2352-2186
negotiable
发表于 2025-3-22 13:42:01
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harangue
发表于 2025-3-22 17:58:09
Disky Ellipticals in the Hubble Sequencehas been suggested that disky ellipticals form together with S0s and spirals a continuous transition in D/B ratio in the Hubble sequence (Bender 1988b, Nieto 1988). However, until the present, this hypothesis had not been investigated throughout.
Type-1-Diabetes
发表于 2025-3-22 23:12:44
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Palpable
发表于 2025-3-23 04:10:27
Population Synthesis Models formation rate (SFR); and . the rate of chemical enrichment (in some models ...). Most of the recent codes use the isochrone synthesis algorithm, which allows to compute the evolution of a simple stellar population (SSP), and from it, by a convolution integral, the properties of more complex composite stellar populations (CSP).
Engaged
发表于 2025-3-23 06:53:37
Recent Progress in the Search for Black Holes in Galactic Nucleiremarkably well. N-body simulations of an edge-on .(..) model for M32 show that this model is stable. HST spectra should soon provide new and improved constraints on the presence of BHs in quiescent galaxies.