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Bintang deret utama tipe-A

Sebuah gambar seniman tentang Sirius A dan Sirius B, sebuah sistem bintang biner. Sirius A, bintang deret utama tipe A, berukuran lebih besar dari yang kedua.

Bintang deret utama tipe A (A V) atau bintang katai A adalah sebuah bintang deret utama (pembakaran hidrogen) bertipe spektrum A dan kelas luminositas V. Bintang-bintang tersebut memiliki spektrum yang ditentukan oleh garis absorpsi hidrogen Balmer.[1][2][3]

Referensi

[sunting | sunting sumber]
  1. ^ Stellar Spectral Types, entry at hyperphysics.phy-astr.gsu.edu, accessed on line June 19, 2007.
  2. ^ "An Introduction to Modern Astrophysics" by B.W Caroll and D.A Ostlie 1996 edition, chapter 8
  3. ^ Adelman, S. J. (2005). "The physical properties of normal A stars". Proceedings of the International Astronomical Union. 2004: 1–11. Bibcode:2004IAUS..224....1A. doi:10.1017/S1743921304004314alt=Dapat diakses gratis. 


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Bintang deret utama tipe-A
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