Chemical Galaxy

Results: 29



#Item
11Dust and Chemical Abundances of the Sagittarius Dwarf Galaxy Planetary Nebula Hen2-436 OTSUKA, Masaaki, MEIXNER, Margaret

Dust and Chemical Abundances of the Sagittarius Dwarf Galaxy Planetary Nebula Hen2-436 OTSUKA, Masaaki, MEIXNER, Margaret

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Source URL: www.nao.ac.jp

Language: English - Date: 2012-07-25 04:23:23
12Extremely metal poor stars and Chemical Evolution in the Early Universe KOMIYA, Yutaka

Extremely metal poor stars and Chemical Evolution in the Early Universe KOMIYA, Yutaka

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Source URL: www.nao.ac.jp

Language: English - Date: 2012-07-25 04:23:22
13Counting Atoms in a Molecule The complex molecule Propanal was discovered in a dense interstellar cloud called Sagittarius B2(North) located near the center of the Milky Way galaxy about 26,000 light years

Counting Atoms in a Molecule The complex molecule Propanal was discovered in a dense interstellar cloud called Sagittarius B2(North) located near the center of the Milky Way galaxy about 26,000 light years

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Source URL: spacemath.gsfc.nasa.gov

Language: English - Date: 2009-04-20 11:45:10
14The chemical evolution of the Local  Group dwarf galaxies as seen by  Gemini+GMOS Denise R. Gonçalves Observatório do Valongo Universidade Federal do Rio de Janeiro, Brazil

The chemical evolution of the Local  Group dwarf galaxies as seen by  Gemini+GMOS Denise R. Gonçalves Observatório do Valongo Universidade Federal do Rio de Janeiro, Brazil

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Source URL: www.gemini.edu

Language: English - Date: 2012-08-03 20:59:47
15GSMT Science Use Case Title: The Star Formation Histories of Disk Galaxies Authors: Olsen, K. Abstract: We describe a program to measure the star formation and chemical enrichment histories of the bulges and disks in a s

GSMT Science Use Case Title: The Star Formation Histories of Disk Galaxies Authors: Olsen, K. Abstract: We describe a program to measure the star formation and chemical enrichment histories of the bulges and disks in a s

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Source URL: www.gsmt.noao.edu

Language: English - Date: 2008-05-06 14:30:01
16The Assembly and Chemical Evolution of Nearby Early-type Galaxies Caroline Foster Presented in fulfillment of the requirements of the degree of Doctor of Philosophy July 2011

The Assembly and Chemical Evolution of Nearby Early-type Galaxies Caroline Foster Presented in fulfillment of the requirements of the degree of Doctor of Philosophy July 2011

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Source URL: www.carofoster.com

Language: English - Date: 2014-07-22 19:12:32
17Counting Atoms in a Molecule The complex molecule Propanal was discovered in a dense interstellar cloud called Sagittarius B2(North) located near the center of the Milky Way galaxy about 26,000 light years

Counting Atoms in a Molecule The complex molecule Propanal was discovered in a dense interstellar cloud called Sagittarius B2(North) located near the center of the Milky Way galaxy about 26,000 light years

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Source URL: spacemath.gsfc.nasa.gov

Language: English - Date: 2009-04-20 12:45:10
18Groups, Clusters and Individuals Astronomers study many different kinds of objects in space. Sometimes these objects contain many individuals that need to be tallied separately. The cluster of galaxies called Abell2218 i

Groups, Clusters and Individuals Astronomers study many different kinds of objects in space. Sometimes these objects contain many individuals that need to be tallied separately. The cluster of galaxies called Abell2218 i

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Source URL: spacemath.gsfc.nasa.gov

Language: English - Date: 2010-05-02 04:17:40
19Star Formation and Chemical Abundances in the Outer Disks and Halos of Galaxies Maria T. Patterson NMSU Astronomy

Star Formation and Chemical Abundances in the Outer Disks and Halos of Galaxies Maria T. Patterson NMSU Astronomy

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Source URL: www.nmspacegrant.com

Language: English - Date: 2011-04-28 15:48:04
20Giant Gas Cloud in System NGC[removed]Scientists have used Chandra to make a detailed study of an enormous cloud of hot gas enveloping two large, colliding galaxies. This unusually large reservoir of gas contains as much m

Giant Gas Cloud in System NGC[removed]Scientists have used Chandra to make a detailed study of an enormous cloud of hot gas enveloping two large, colliding galaxies. This unusually large reservoir of gas contains as much m

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Source URL: www.chandra.harvard.edu

Language: English - Date: 2013-05-10 10:31:36