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Physics 231: Section 6 Galaxies. http:// mimas.physics.drexel.edu /phys231. M104 – The “Sombrero” Galaxy. Sa Galaxy Very prominent bulge with tightly wound spiral arms. M81 . Sb galaxy. Extended bulge but with relatively prominent arms. M74. Sc galaxy Tight galactic bulge.
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Physics 231: Section 6Galaxies http://mimas.physics.drexel.edu/phys231 Phys 231, Topic 6: Galaxies
M104 – The “Sombrero” Galaxy Sa Galaxy Very prominent bulge with tightly wound spiral arms Phys 231, Topic 6: Galaxies
M81 Sb galaxy. Extended bulge but with relatively prominent arms. Phys 231, Topic 6: Galaxies
M74 Sc galaxy Tight galactic bulge. Very extended, blue arms. Phys 231, Topic 6: Galaxies
Stellar mass function in galaxies. From Pannella et al. (2009) Red=“Early Type” Blue=“Late Type” Phys 231, Topic 6: Galaxies
M102 A “Lenticular” galaxy Phys 231, Topic 6: Galaxies
M109 SBc Barred Spiral Phys 231, Topic 6: Galaxies
M59 An E5 galaxy. Phys 231, Topic 6: Galaxies
Sextans A Irregular galaxy Phys 231, Topic 6: Galaxies
Morphological Segregation From Dominguez et al. (2000). Spirals and Irregulars (S+I) preferentially live in low density environments. Early types (Ellipticalsand S0’s) live in high density environments. Phys 231, Topic 6: Galaxies
Which one is another galaxy, and which one is part of the Milky Way? Phys 231, Topic 6: Galaxies
The Globular Cluster M13 Phys 231, Topic 6: Galaxies
Cepheid Variables Phys 231, Topic 6: Galaxies
Rotation Curve of NGC891 (in HI) Phys 231, Topic 6: Galaxies
Herschel/Kapteyn Model of the Milky Way (with the sun near the center) Phys 231, Topic 6: Galaxies
The Structure of the Milky Way Phys 231, Topic 6: Galaxies
Black Hole/Bulge Relation Phys 231, Topic 6: Galaxies
Coma Cluster (optical) Phys 231, Topic 6: Galaxies
Coma Cluster (X-ray) Phys 231, Topic 6: Galaxies
Hubble’s Original Measurement Phys 231, Topic 6: Galaxies