找回密码
 To register

QQ登录

只需一步,快速开始

扫一扫,访问微社区

Titlebook: Dense Molecular Gas around Protostars and in Galactic Nuclei; European Workshop on W.A. Baan,Y. Hagiwara,H.J. Langevelde Book 2005 Springer

[复制链接]
楼主: 叛乱分子
发表于 2025-3-28 15:08:53 | 显示全部楼层
A Molecular Ring in the Liner NGC 5218entration with extensions out to a radius of 12″. The molecular mass detected is 2.4 × 10. . and the gas surface density is high, ∼3000 . pc square in the inner 500 pc. The SFR is 2–3 . yr . and the SFE is ∼13, which are low or moderate values for that gas surface density. We interpret the inner fea
发表于 2025-3-28 20:15:22 | 显示全部楼层
发表于 2025-3-29 00:57:43 | 显示全部楼层
discussed here are often in an early stage and undoubtedly their progress has bene?ted greatly from the opportunity to discuss results with the experts in a wide range of areas. Similarly, we feel con?dent tha978-90-481-6772-2978-1-4020-3831-0
发表于 2025-3-29 03:52:19 | 显示全部楼层
Domestic Dog Cognition and Behavior activity. The overall lack of observational evidence for direct causal relationships between the presence of bars and interactions on the one hand, and starburst or Seyfert activity on the other could, however, easily be due to the possibility that we are not yet considering the correct spatial- or
发表于 2025-3-29 10:37:13 | 显示全部楼层
https://doi.org/10.1007/978-3-642-53994-7ibution caused by orbit crowding effects. Based on these new data we have improved recent simulations of the warped disk in NGC3718. HE1029-1831 and 3C48 are nearby QSOs. HE10297-1831 is taken out of the Cologne nearby QSO sample. The maps of the integrated CO(1-0) and CO(2–1) emission clearly show
发表于 2025-3-29 11:46:02 | 显示全部楼层
EVN Observations of H2O Masers Towards the High-Mass Young Stellar Object in AFGL 5142
发表于 2025-3-29 15:42:36 | 显示全部楼层
Dense Molecular Gas around Protostars and in Galactic NucleiEuropean Workshop on
发表于 2025-3-29 19:42:33 | 显示全部楼层
Dense Molecular Gas around Protostars and in Galactic Nuclei978-1-4020-3831-0
发表于 2025-3-30 03:06:49 | 显示全部楼层
Gravitationally Induced Inflow in Starbursts and AGN activity. The overall lack of observational evidence for direct causal relationships between the presence of bars and interactions on the one hand, and starburst or Seyfert activity on the other could, however, easily be due to the possibility that we are not yet considering the correct spatial- or
发表于 2025-3-30 05:16:00 | 显示全部楼层
 关于派博传思  派博传思旗下网站  友情链接
派博传思介绍 公司地理位置 论文服务流程 影响因子官网 SITEMAP 大讲堂 北京大学 Oxford Uni. Harvard Uni.
发展历史沿革 期刊点评 投稿经验总结 SCIENCEGARD IMPACTFACTOR 派博系数 清华大学 Yale Uni. Stanford Uni.
|Archiver|手机版|小黑屋| 派博传思国际 ( 京公网安备110108008328) GMT+8, 2025-5-19 22:08
Copyright © 2001-2015 派博传思   京公网安备110108008328 版权所有 All rights reserved
快速回复 返回顶部 返回列表