'Absolute magnitudes' presentation slideshows

The Milky Way

The Milky Way. Our home galaxy, full of stars, gas and mysterious dark matter We decompose it into a disk and a halo and a few other parts. Second Exam Results. Mean: 53.7 + 20 pt curve = 73.9 Standard deviation: 10.4 Maximum: 76 raw, 92 curved ; Minimum: 36 raw, 56 curved.

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Morphological Classification

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1B11 Foundations of Astronomy Star names and magnitudes

1B11 Foundations of Astronomy Star names and magnitudes. Liz Puchnarewicz emp@mssl.ucl.ac.uk www.ucl.ac.uk/webct www.mssl.ucl.ac.uk/. 1B11 Our night sky.

483 views • 31 slides

Stars and Nebulae

Stars and Nebulae. The study of the stars & nebulae provides information about the origin and history of the Earth and the solar system. Astronomers discover how stars like our Sun are born, grow old and die. Review. Pulsars are ...like neutron stars because....

427 views • 29 slides

FT228/4 Knowledge Based Decision Support Systems

483 views • 22 slides

The Sun, the closest star

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335 views • 21 slides

CAPSTONE Lecture 6 HR Diagram

CAPSTONE Lecture 6 HR Diagram. Two stars at distances d 1 and d 2 with intrinsic total luminosities L 1 and L 2 . (L=4 p r 2 s T 4 ). Flux, f , is ergs per cm squared per second over some frequency interval is received at Earth.

168 views • 16 slides

New Analysis of Open Clusters Using CCD Photometry

New Analysis of Open Clusters Using CCD Photometry. Kayla Young. Future Studies. Add more Open Clusters to compare more ages and absolute magnitude. Using a CCD Imager and B and V filters take images of clusters, instead of downloading them.

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ABSTRACT:

Infrared Studies of Type Ia Supernovae. M. Verdugo O. (PUC), K. Krisciunas (CTIO/OCIW), N. B. Suntzeff (CTIO), M. M. Phillips (OCIW), P. Candia (CTIO). ABSTRACT:

111 views • 1 slides