Volume 438, Number 2, August I 2005
|Page(s)||L21 - L24|
|Published online||08 July 2005|
Letter to the Editor
On the origin of the X-ray emission towards the early Herbig Be star MWC 297
Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, UK e-mail: email@example.com
2 California Institute of Technology, Mail Code 102-8, 1200 E. California Blvd., Pasadena CA 91125, USA
Accepted: 12 June 2005
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.
Key words: stars: formation / stars: pre-main sequence / stars: flare / stars: individual: M 297 / X-rays: stars
© ESO, 2005
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