sfr in high redshift clusters with spitzer

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SFR in High Redshift Clusters with Spitzer By Vinay Patel

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Page 1: Sfr In High Redshift Clusters With Spitzer

SFR in High Redshift Clusters with Spitzer

By

Vinay Patel

Page 2: Sfr In High Redshift Clusters With Spitzer

The Formation of Stars

Interstellar Medium Clumps of Gas and Dust Gravity’s Effect Protostar Hydrogen Fusion Solar Wind

Page 4: Sfr In High Redshift Clusters With Spitzer

What Is SFR?

SFR = Star Formation Rate Solar Masses Per Year Variable Usage Varies Depending on Position

Page 5: Sfr In High Redshift Clusters With Spitzer

Measurement of SFR

Total Infrared Luminosity (LTIR)

Spectral Energy Distributions (SEDs) 5 Models Different ‘c’ Values

Two Equations: LTIR(galaxy) = c x L15(galaxy)

SFR(Mо yr-1) = 4.5 x 10-44 x LTIR(erg s-1)

Page 6: Sfr In High Redshift Clusters With Spitzer

Spitzer’s Use

Uses Infrared Technology Infrared is Heat Radiation Wavelength Longer than

Visible Light Interstellar Medium

Dust and Gas Invisible Regions Become

Visible

Page 8: Sfr In High Redshift Clusters With Spitzer

Cluster 1037-1243

Average SFR Per Cluster Member: 60.47 Mо/yr

Total SFR for Cluster: 1693 Mо/yr

Page 9: Sfr In High Redshift Clusters With Spitzer
Page 10: Sfr In High Redshift Clusters With Spitzer
Page 11: Sfr In High Redshift Clusters With Spitzer

The Future

CL1037 Is One of Three Clusters More Data to Come Gain Insights to Galaxy

Evolution