Herbig Ae/Be star

Rarity: Uncommon

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What Wikipedia says

A Herbig Ae/Be star (HAeBe) is a pre-main-sequence star – a young (<10 Myr) star of spectral types A or B. These stars are still embedded in gas-dust envelopes and are sometimes accompanied by circumstellar disks. Hydrogen and calcium emission lines are observed in their spectra.

Excerpt from the Wikipedia article “Herbig Ae/Be star”, under the CC BY-SA 4.0 license. Read the article on Wikipedia

Image: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration, Public domain, via Wikimedia Commons.