Details

Autor(en) / Beteiligte

• Pease, Deron O
• Drake, Jeremy J
• Kashyap, Vinay L

Titel

The Darkest Bright Star: Chandra X-Ray Observations of Vega

Ist Teil von

• The Astrophysical journal, 2006-01, Vol.636 (1), p.426-431

Ort / Verlag

Chicago, IL: IOP Publishing

Erscheinungsjahr

2006

Quelle

EZB Free E-Journals

Beschreibungen/Notizen

• We present X-ray observations of Vega obtained with the Chandra High Resolution Camera and Advanced CCD Imaging Spectrometer. After a total of 29 ks of observation with Chandra, X-rays from Vega remain undetected. We derive upper limits to the X-ray luminosity of Vega as a function of temperature over the range of 10 super(5)-10 super(7) K and find a 99.7% upper limit as low as 62 x 10 super(25) ergs s super(-1) at T = 10 super(6.2) K. We also compare these new deeper observations with the limit derived from a reanalysis of ROSAT PSPC data. Our X-ray luminosity limit for Vega is still greater than predictions of post-Herbig Ae phase X-rays from the shear dynamo model proposed by Tout & Pringle for a Vega age of 350 Myr. If the age of Vega is closer to 100 Myr, as suggested by some indicators, our X-ray limit is then similar to Tout-Pringle model predictions. Current X-ray observations of Vega are therefore unable to discriminate between different scenarios explaining the X-ray activity of the convectively stable Herbig Ae/Be stars. Further progress is more likely to be achieved through X-ray observations of younger main-sequence early-type A stars, whose conjectured residual post-Herbig Ae phase X-ray activity would be significantly higher.