适婚女孩
发表于 2025-3-21 16:59:38
书目名称Open Issues in Local Star Formation影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0701808<br><br> <br><br>书目名称Open Issues in Local Star Formation影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0701808<br><br> <br><br>书目名称Open Issues in Local Star Formation网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0701808<br><br> <br><br>书目名称Open Issues in Local Star Formation网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0701808<br><br> <br><br>书目名称Open Issues in Local Star Formation被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0701808<br><br> <br><br>书目名称Open Issues in Local Star Formation被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0701808<br><br> <br><br>书目名称Open Issues in Local Star Formation年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0701808<br><br> <br><br>书目名称Open Issues in Local Star Formation年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0701808<br><br> <br><br>书目名称Open Issues in Local Star Formation读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0701808<br><br> <br><br>书目名称Open Issues in Local Star Formation读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0701808<br><br> <br><br>
Mingle
发表于 2025-3-21 22:48:49
978-90-481-6489-9Springer Science+Business Media Dordrecht 2003
JIBE
发表于 2025-3-22 03:19:22
Open Issues in Local Star Formation978-1-4020-2600-3Series ISSN 0067-0057 Series E-ISSN 2214-7985
主动
发表于 2025-3-22 07:46:36
0067-0057 Overview: 978-90-481-6489-9978-1-4020-2600-3Series ISSN 0067-0057 Series E-ISSN 2214-7985
NOTCH
发表于 2025-3-22 11:23:39
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/o/image/701808.jpg
保存
发表于 2025-3-22 13:40:39
https://doi.org/10.1007/1-4020-2600-5Accretion; Main sequence; X-ray; relativistic jet; solar; star; stars; stellar
松软
发表于 2025-3-22 19:38:01
http://reply.papertrans.cn/71/7019/701808/701808_7.png
矛盾心理
发表于 2025-3-23 00:02:13
http://reply.papertrans.cn/71/7019/701808/701808_8.png
NIP
发表于 2025-3-23 04:31:12
http://reply.papertrans.cn/71/7019/701808/701808_9.png
Ligneous
发表于 2025-3-23 07:06:11
Classification of the Pico Dos Dias Survey Herbig Ae/Be Starsted S., the contribution of the circumstellar components (dust disk and/or envelope) to the total emitted flux. We classified the sample stars in 3 groups based on the shape of their SEDs. We analyzed this classification and S. in relation to other properties of the these stars.