Presentation is loading. Please wait.

Presentation is loading. Please wait.

Surface Brightness Profile - NGC 3379 (giant elliptical)

Similar presentations


Presentation on theme: "Surface Brightness Profile - NGC 3379 (giant elliptical)"— Presentation transcript:

1 Surface Brightness Profile - NGC 3379 (giant elliptical)
Surface Brightness (mags/arcsec2) Dashed line is a deV law r1/4

2 King Models - A Family of Curves
deV law would be a straight line on this plot Note: “Isothermal” sphere is classic model where density is r( r ) ~ 1/r2 Surface Brightness r1/4

3 Error Function

4

5 King Models and Observed Objects
NGC 6388 Circles: globular cluster NGC 6388 Squares: globular cluster NGC 5053 Triangles: Sculptor dwarf galaxy NGC 5053 Sculptor Dwarf Galaxy

6 Giant Elliptical NGC 4472 (c = 2.35)
SDSS image Solid line is King Model with c = 2.35

7 deV vs. King: NGC 3379 Dots: observations Dashed line: deV law
Solid line: King model, c = 2.2

8 Two Galaxies in Same Cluster: Dwarf E and Giant E
Dashed - Giant E, r1/4 Solid - Dwarf E, exp[-r/rs]

9 cD Galaxy - The Biggest of the Big
Line: deV Line: deV law ?

10 Schechter Luminosity Function
The most intrinsically luminous galaxies are primarily red in color and are rare The most intrinsically faint galaxies are the most numerous and are primarily blue in color (irregulars vastly outnumber dwarf E) blue red

11 “Violent Relaxation” of Star Cluster
“cold” start minimum size maximum size end

12 Density Profile: Before and After Violent Relaxation
Uniform density sphere (dashed line) at start R1/4 law at end (squares + solid line)

13 Distribution of Stellar Energies: Before, During, and after Violent Relaxation
start end


Download ppt "Surface Brightness Profile - NGC 3379 (giant elliptical)"

Similar presentations


Ads by Google