Optical spectroscopy of an m-type star / Arrief Azzahir Daud

Daud, Arrief Azzahir (2008) Optical spectroscopy of an m-type star / Arrief Azzahir Daud. [Student Project] (Unpublished)

Download

[thumbnail of 43810.pdf] Text
43810.pdf

Download (115kB)

Abstract

In this research, the researcher performs the astronomical spectroscopy of an M-type star aided by 20 inch telescope, CCD and spectrograph. The researcher were successfully obtained absorption lines spectrum of the M-type star (Betelgeuse) at 3 different ranges and exposure time. Analysis of the M-type star spectrum resulting 7 TiO (at 5409.483, 5823.811, 5753.659, 6126.678, 6181.934, 6221.255, 6326.464 A), 3 Fe (at 5806.795, 6412.544, 6422.108 A) and 2 Nal (at 5890.018, 5896.425 A) absorption lines were identified in the M-type star spectrum. Analysis also shows that the radial velocity of the stars on the night of observation (22nd to 28™ December 2007 at LNO) was +29.121 x 103 m/s means that the star was moving away from earth. The error in obtaining the spectra were reduced by lowering the CCD's temperature, subtracting the dark current and flat fielding the image obtained.

Metadata

Item Type: Student Project
Creators:
Creators
Email
Daud, Arrief Azzahir
UNSPECIFIED
Contributors:
Contribution
Name
Email / ID Num.
Thesis advisor
Mohamad, Siti Jamiah
UNSPECIFIED
Subjects: R Medicine > RE Ophthalmology
Divisions: Universiti Teknologi MARA, Shah Alam > Faculty of Applied Sciences
Programme: Degree of Bachelor of Science (Hons.) Physic
Item ID: 43810
Uncontrolled Keywords: Optical, spectroscopy, spectrum
URI: https://ir.uitm.edu.my/id/eprint/43810

Fulltext

Fulltext is available at:
  • Koleksi Akses Terhad | PTAR Utama | Shah Alam
  • ID Number

    43810

    Indexing


    View in Google Scholar

    Edit Item
    Edit Item