Explore: Disk Galaxies
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Books Results
Source: The Open Library
The Open Library Search Results
Search results from The Open Library
1A2111, a z = 0.23 Butcher-Oemler cluster with a non-isothermal atmosphere and normal metallicity
By Q. Daniel Wang
“A2111, a z = 0.23 Butcher-Oemler cluster with a non-isothermal atmosphere and normal metallicity” Metadata:
- Title: ➤ A2111, a z = 0.23 Butcher-Oemler cluster with a non-isothermal atmosphere and normal metallicity
- Author: Q. Daniel Wang
- Language: English
- Publisher: ➤ National Technical Information Service, distributor - National Aeronautics and Space Administration
- Publish Date: 1998
- Publish Location: ➤ Springfield, Va - [Washington, DC
“A2111, a z = 0.23 Butcher-Oemler cluster with a non-isothermal atmosphere and normal metallicity” Subjects and Themes:
- Subjects: ➤ Astrophysics - Disk galaxies - Galactic clusters - Intergalactic media - Metallicity - Proportional counters - ROSAT mission - X rays
Edition Identifiers:
- The Open Library ID: OL17595612M - OL17133279M - OL18134458M - OL15546996M
- Online Computer Library Center (OCLC) ID: 42075899
Access and General Info:
- First Year Published: 1998
- Is Full Text Available: No
- Is The Book Public: No
- Access Status: No_ebook
Online Access
Downloads Are Not Available:
The book is not public therefore the download links will not allow the download of the entire book, however, borrowing the book online is available.
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2Excitation and evolution of structure in galaxies (NAG 5-2873)
By Martin D. Weinberg
“Excitation and evolution of structure in galaxies (NAG 5-2873)” Metadata:
- Title: ➤ Excitation and evolution of structure in galaxies (NAG 5-2873)
- Author: Martin D. Weinberg
- Language: English
- Publisher: ➤ National Technical Information Service, distributor - National Aeronautics and Space Administration
- Publish Date: 1996
- Publish Location: ➤ Springfield, Va - [Washington, DC
“Excitation and evolution of structure in galaxies (NAG 5-2873)” Subjects and Themes:
- Subjects: Disk galaxies - A stars - Amplification - Galactic evolution - Excitation
Edition Identifiers:
- The Open Library ID: OL15547441M
Access and General Info:
- First Year Published: 1996
- Is Full Text Available: No
- Is The Book Public: No
- Access Status: No_ebook
Online Access
Downloads Are Not Available:
The book is not public therefore the download links will not allow the download of the entire book, however, borrowing the book online is available.
Online Borrowing:
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3A 21 centimeter absorber identified with a spiral galaxy
“A 21 centimeter absorber identified with a spiral galaxy” Metadata:
- Title: ➤ A 21 centimeter absorber identified with a spiral galaxy
- Language: English
- Publisher: ➤ National Aeronautics and Space Administration - National Technical Information Service, distributor
- Publish Date: 1996
- Publish Location: ➤ [Washington, DC - Springfield, Va
“A 21 centimeter absorber identified with a spiral galaxy” Subjects and Themes:
- Subjects: ➤ Hubble Space Telescope - Luminosity - Spiral galaxies - Line spectra - Faint objects - Barred galaxies - Disk galaxies - Imaging techniques
Edition Identifiers:
- The Open Library ID: OL17837673M
- Online Computer Library Center (OCLC) ID: 40532368
Access and General Info:
- First Year Published: 1996
- Is Full Text Available: No
- Is The Book Public: No
- Access Status: No_ebook
Online Access
Downloads Are Not Available:
The book is not public therefore the download links will not allow the download of the entire book, however, borrowing the book online is available.
Online Borrowing:
Online Marketplaces
Find A 21 centimeter absorber identified with a spiral galaxy at online marketplaces:
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- Ebay: New & used books.
Wiki
Source: Wikipedia
Wikipedia Results
Search Results from Wikipedia
Disc galaxy
with other nearby galaxies can perturb and stretch the galactic disk. Disc galaxy types include: Spiral galaxies: Unbarred spiral galaxies: (types S, SA)
Lenticular galaxy
E galaxies with the S0 galaxies are the ES galaxies with intermediate-scale discs. Lenticular galaxies are unique in that they have a visible disk component
Thick disk
The thick disk is one of the structural components of about 2/3 of all disk galaxies, including the Milky Way. It was discovered first in external edge-on
Galaxy formation and evolution
first galaxies, the way galaxies change over time, and the processes that have generated the variety of structures observed in nearby galaxies. Galaxy formation
Galactic bulge
the center of most spiral galaxies. Bulges were historically thought to be elliptical galaxies that happened to have a disk of stars around them, but
Elliptical galaxy
Elliptical (E) galaxies are, together with lenticular galaxies (S0) with their large-scale disks, and ES galaxies with their intermediate scale disks, a subset
Spiral galaxy
as such, form part of the Hubble sequence. Most spiral galaxies consist of a flat, rotating disk containing stars, gas and dust, and a central concentration
Milky Way
light-years (613 kpc). The Milky Way has several satellite galaxies and is part of the Local Group of galaxies, forming part of the Virgo Supercluster which is
Thin disk
The thin disk is a structural component of spiral and S0-type galaxies, composed of stars, gas and dust. It is the main non-centre (e.g. galactic bulge)
Dead disk
dead disk galaxy is a type of galaxy that is no longer able to form new stars. These galaxies are usually massive yet compact, fast spinning disk shaped