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Titlebook: Cores to Clusters; Star Formation with M. S. N. Kumar,M. Tafalla,P. Caselli Conference proceedings 2005 Springer-Verlag New York 2005 Astr

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樓主: HAVEN
11#
發(fā)表于 2025-3-23 11:25:18 | 只看該作者
Preliminary Results on Newly Discovered Embedded Clustersnitude. To date we have observed 25 of the 346 clusters found by Bica and Dutra (2003). We constructed near-IR color-color diagrams to identify PMS stars in the clusters and examined the distribution of these stars in the cluster field. In this proceeding we show the results concerning three candidates of our survey.
12#
發(fā)表于 2025-3-23 14:10:06 | 只看該作者
13#
發(fā)表于 2025-3-23 21:24:25 | 只看該作者
14#
發(fā)表于 2025-3-23 23:40:45 | 只看該作者
15#
發(fā)表于 2025-3-24 03:28:08 | 只看該作者
16#
發(fā)表于 2025-3-24 09:18:35 | 只看該作者
0067-0057 er and millimeter wave bands will become operationalIt was with pleasure that CAUP became for three days the core to the cloud of star formation experts all over the world. Close to the celebration of its 15th anniversary – therefore still in the early stages of institutional evolution – we are prou
17#
發(fā)表于 2025-3-24 13:52:55 | 只看該作者
18#
發(fā)表于 2025-3-24 16:45:07 | 只看該作者
19#
發(fā)表于 2025-3-24 19:16:13 | 只看該作者
Controlled Singularly Perturbed Systems,ery recently, puts us in a very good position to plan rich and fruitful observative campaigns with the instruments being developed for astronomy at IR, submm amd mm wavelengths, in interferometric or single-telescope modes.
20#
發(fā)表于 2025-3-25 00:36:08 | 只看該作者
Management of Radioactive Wastes,d is not affected by the problems mentioned above, which makes it a privileged target for studying not only PMS evolution and BDs but also offers a valuable opportunity to study the IMF well down into the substellar regime.
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