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Dorado constellation Large Magellanic Cloud Celestial mechanics Rotational energy Angular momentum Rigid body dynamics Retrograde motion Star Rotational speed Physics Rotational symmetry Physical quantities | Astronomy & Astrophysics A&A 545, L1DOI:Add to Reading ListSource URL: www.aanda.orgDownload Document from Source WebsiteFile Size: 298,11 KBShare Document on Facebook |
Proposal to establish a DFG priority program Physics of the Interstellar Medium Figure 1: This figure shows the star forming region NGC 602 in the Large Magellanic Cloud. Potsdam University leads a large observational pDocID: 1tQdG - View Document | |
X-Ray View of A Thousand-Year-Old Cosmic TapestryDocID: 1rc5g - View Document | |
Chandra Observations of SN 1987A Kari A. Frank with David BurrowsDocID: 1qmq5 - View Document | |
Page: 1 Slide No. 1 Stars of the Universe How stars are bornDocID: 1oNPi - View Document | |
The VVV Survey reveals classical Cepheids tracing a young and thin stellar disk across the Galaxy’s bulge I. D´ek´any1,2 , D. Minniti3,1,4 , D. Majaess5,6 , M. Zoccali2,1 , G. Hajdu2,1 , J. Alonso-Garc´ıa7,1 , M. CDocID: 1onRg - View Document |