P. Manoj, G. Maheswar, H. C. Bhatt
Abstract
Pre-main sequence stars of intermediate mass (2 ≤ M/M ⊙ ≤ 8) which show emission lines in their spectra are called Herbig Ae/Be (HAEBE) stars. They were first discussed as a group by Herbig (1960). He identified 26 stars
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Pre-main sequence stars of intermediate mass (2 ≤ M/M ⊙ ≤ 8) which show emission lines in their spectra are called Herbig Ae/Be (HAEBE) stars. They were first discussed as a group by Herbig (1960). He identified 26 stars
Key concepts: Physics, Astrophysics, Stars, Herbig Ae/Be star, Orion Nebula, Nebula, Circumstellar dust, Astronomy