Stellar kinematics

Results: 44



#Item
21Sloan Extension for Galactic Underpinnings and Evolution (SEGUE) Segue (v.): To proceed to what follows without pause Heidi Newberg1 , Kurt Anderson2,3 , Timothy Beers4 , Jon Brinkmann3 , Bing Chen5 , Eva Grebel6 , ˇ Ji

Sloan Extension for Galactic Underpinnings and Evolution (SEGUE) Segue (v.): To proceed to what follows without pause Heidi Newberg1 , Kurt Anderson2,3 , Timothy Beers4 , Jon Brinkmann3 , Bing Chen5 , Eva Grebel6 , ˇ Ji

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Source URL: classic.sdss.org

Language: English - Date: 2014-04-01 14:25:55
22Stellar astronomy / Galactic astronomy / Globular clusters / Local Group / 47 Tucanae / Blue straggler / Cosmic distance ladder / Star / Stellar kinematics / Astronomy / Space / Star clusters

HEIC0616: FOR IMMEDIATE RELEASE 16:00 (CEST)/10:00 AM EDT 24 October, 2006

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Source URL: www.spacetelescope.org

Language: English - Date: 2006-10-24 09:51:37
23Microsoft Word - heic0616_vip.doc

Microsoft Word - heic0616_vip.doc

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Source URL: www.spacetelescope.org

Language: English - Date: 2006-10-24 10:03:13
24The Astrophysical Journal, 631:280–300, 2005 September 20 # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. HST STIS SPECTROSCOPY OF THE TRIPLE NUCLEUS OF M31: TWO NESTED DISKS IN KEPLER

The Astrophysical Journal, 631:280–300, 2005 September 20 # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. HST STIS SPECTROSCOPY OF THE TRIPLE NUCLEUS OF M31: TWO NESTED DISKS IN KEPLER

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Source URL: chandra.as.utexas.edu

Language: English - Date: 2005-09-21 12:13:29
25Jessica Ryan Lu Contact Information Institute for Astronomy University of Hawaii

Jessica Ryan Lu Contact Information Institute for Astronomy University of Hawaii

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Source URL: www.ifa.hawaii.edu

Language: English - Date: 2014-07-29 16:14:50
26June Sky - East  Musca 60° 0°

June Sky - East Musca 60° 0°

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Source URL: home.mira.net

Language: English - Date: 2014-05-27 10:06:53
27Chapter 2  Populations and Components of the Milky Way Our perspective from within the Milky Way gives us an opportunity to study a disk galaxy in detail. At the same time, it’s not always easy to relate what we find i

Chapter 2 Populations and Components of the Milky Way Our perspective from within the Milky Way gives us an opportunity to study a disk galaxy in detail. At the same time, it’s not always easy to relate what we find i

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Source URL: www.ifa.hawaii.edu

Language: English - Date: 2009-01-25 16:42:50
28Chapter 15  Kinematics of the Solar Neighborhood Unlike an elliptical galaxy, the Milky Way rotates with a speed much larger than the random velocities of typical stars. Our position inside the disk of the Milky Way is b

Chapter 15 Kinematics of the Solar Neighborhood Unlike an elliptical galaxy, the Milky Way rotates with a speed much larger than the random velocities of typical stars. Our position inside the disk of the Milky Way is b

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Source URL: www.ifa.hawaii.edu

Language: English - Date: 2009-03-30 21:33:43
29Star Clusters  Star Clusters

Star Clusters Star Clusters

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Source URL: www.astro.caltech.edu

Language: English - Date: 2004-11-17 19:55:28
30Star formation in unbound giant molecular clouds: the origin of OB associations?

Star formation in unbound giant molecular clouds: the origin of OB associations?

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Source URL: mnras.oxfordjournals.org

Language: English