SIMBAD references

2004ApJ...614..221S - Astrophys. J., 614, 221-234 (2004/October-2)

New perspectives on the X-ray emission of HD 104237 and other nearby Herbig Ae/Be stars from XMM-newton and Chandra.

SKINNER S.L., GUDEL M., AUDARD M. and SMITH K.

Abstract (from CDS):

The origin of the X-ray emission from Herbig Ae/Be stars is not yet known. These intermediate-mass pre-main-sequence stars lie on radiative tracks and are not expected to emit X-rays via solar-like magnetic processes, nor are their winds powerful enough to produce X-rays by radiative wind shocks as in more massive O-type stars. The emission could originate in unseen low-mass companions, or it may be intrinsic to the Herbig stars themselves if they still have primordial magnetic fields or can sustain magnetic activity via a nonsolar dynamo. We present new X-ray observations of the nearby Herbig Ae star HD 104237 (=DX Cha) with XMM-Newton, whose objective is to clarify the origin of the emission. Several X-ray emission lines are clearly visible in the CCD spectra, including the high-temperature Fe Kα complex. The emission can be accurately modeled as a multitemperature thermal plasma with cool (kT<1 keV) and hot (kT≳3 keV) components. The presence of a hot component is compelling evidence that the X-rays originate in magnetically confined plasma, either in the Herbig star itself or in the corona of an as yet unseen late-type companion. The X-ray temperatures and luminosity (logLX=30.5 ergs/s) are within the range expected for a T Tauri companion, but high-resolution Chandra and Hubble Space Telescope images constrain the separation of a putative companion to less than 1". We place these new results into broader context by comparing the X-ray and bolometric luminosities of a sample of nearby Herbig stars with those of T Tauri stars and classical main-sequence Be stars. We also test the predictions of a model that attributes the X-ray emission of Herbig stars to magnetic activity that is sustained by a shear-powered dynamo.

Abstract Copyright:

Journal keyword(s): Stars: Emission-Line, Be - Stars: Individual: Henry Draper Number: HD 104237 - Stars: Individual: Henry Draper Number: HD 150193 - Stars: Individual: Henry Draper Number: HD 163296 - Stars: Individual: Constellation Name: R Coronae Australis - Stars: Individual: Constellation Name: T Coronae Australis - Stars: Pre-Main-Sequence - X-Rays: Stars

Nomenclature: Table 3: [SGA2004] NN (Nos 1-19).

Simbad objects: 41

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