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- W2037094585 abstract "We present high resolution (0.2) AO-corrected coronographic near-infrared imaging on the early-type Herbig Be star MWC 297. X-ray flaring has been reported towards this young object, however this has been difficult to reconcile with its early spectral type (B1.5) and relatively high mass (~10 ). Our infrared and X-ray analysis shows that the X-ray flaring is likely due to a late-type star in the same field. The case of MWC 297 emphasizes the need for coronographic imaging to address the reality of X-ray emission towards Herbig Ae/Be stars, which is needed to understand the differences between low and high-mass star formation." @default.
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- W2037094585 date "2005-07-08" @default.
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- W2037094585 title "On the origin of the X-ray emission towards the early Herbig Be star MWC 297" @default.
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- W2037094585 doi "https://doi.org/10.1051/0004-6361:200500141" @default.
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