1 / 9

Sirius A and B

0. Sirius A and B. 0. I l ( t l ) = I l (0) e -h n /kT + B l (T) (1 – e -h n /kT ). 0. Limb Darkening. 0. Structure of Spectral Lines. 0. Equivalent Width. W. 1. 0.8. 0.6. F l /F cont. 0.4. 0.2. l. l 0. 0. Doppler Broadening. Red shifted abs. Blue shifted abs. v r.

Télécharger la présentation

Sirius A and B

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. 0 Sirius A and B

  2. 0 Il (tl) = Il (0) e-hn/kT + Bl(T) (1 – e-hn/kT)

  3. 0 Limb Darkening

  4. 0 Structure of Spectral Lines

  5. 0 Equivalent Width W 1 0.8 0.6 Fl/Fcont 0.4 0.2 l l0

  6. 0 Doppler Broadening Red shifted abs. Blue shifted abs. vr Observer vr Atoms in random thermal motion

  7. 0 Line Profiles Gauss Profile 1 0.8 Lorentz Profile 0.6 Fl/Fcont 0.4 0.2 l l0

  8. 0 Line Profiles Increasing number of absorbing atoms 1 0.8 0.6 Fl/Fcont 0.4 0.2 l l0

  9. 0 Curve of Growth Log(W/l0) ~ √Nfl -4 ~ √log(Nfl) -4.5 -5 ~ Nfl -5.5 11 12 13 14 15 16 Log(Nfl)

More Related