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SLOAN LED 214500 Low-Redshift Analogs of Cosmic Noon Galaxies as Laboratories for Clumpy Star Formation
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- $163.54
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Product DescriptionThe SLOAN LED 214500 analyzes a specific sample of eighteen supercompact ultraviolet luminous galaxies studied with the OSIRIS spectrograph at the Keck Telescope. This investigation targets their Paα emission. These galaxies possess properties akin to star-forming galaxies. The research identifies a total of eighty-four star-forming clumps, each typically measuring a few hundred parsecs in size.
- Analyzes star-forming clumps in low-redshift galaxies.
- Compares properties to galaxies at cosmic noon.
- Simulates high-redshift observations.
Product Highlights
This product offers deep insights into star formation processes within low-redshift galaxies, providing a comparison to historical cosmic phenomena.Product Information
Standard Information
-
Weight: 0.1 pounds
Technical Specifications
-
Sample Size: 18 galaxies
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Research Tool: OSIRIS spectrograph
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Emission Target: Paα
-
Clumps Identified: 84 clumps
-
Typical Clump Size: Few hundred parsecs
- Analyzes star-forming clumps in low-redshift galaxies.
- Compares properties to galaxies at cosmic noon.
- Simulates high-redshift observations.
Product Highlights
This product offers deep insights into star formation processes within low-redshift galaxies, providing a comparison to historical cosmic phenomena.Product Information
Standard Information
- Weight: 0.1 pounds
Technical Specifications
- Sample Size: 18 galaxies
- Research Tool: OSIRIS spectrograph
- Emission Target: Paα
- Clumps Identified: 84 clumps
- Typical Clump Size: Few hundred parsecs
Vendor: SLOAN
SLOAN LED 214500 Low-Redshift Analogs of Cosmic Noon Galaxies as Laboratories for Clumpy Star Formation
$163.54
Vendor: SLOAN
SLOAN LED 214500 Low-Redshift Analogs of Cosmic Noon Galaxies as Laboratories for Clumpy Star Formation
$163.54
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