Catalog Service: HD 50138 short-term variability
Description
HD 50138 presents the B[e] phenomenon, but its nature is not clear yet. This star is known to present spectral variations, which have been associated with outbursts and shell phases. We analyze the line profile variability of HD 50138 and its possible origin, which provide possible hints to its evolutionary stage, so far said to be close to the end of (or slightly beyond) the main sequence.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2012 Nov 12 07:54:34ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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