A Statistical Spectropolarimetric Study of Herbig Ae/Be Stars
arXiv:1707.08408 · doi:10.1093/mnras/stx1891
Abstract
We present Halpha linear spectropolarimetry of a large sample of Herbig Ae/Be stars. Together with newly obtained data for 17 objects, the sample contains 56 objects, the largest such sample to date. A change in linear polarization across the Halpha line is detected in 42 (75 %) objects, which confirms the previous finding that the circumstellar environment around these stars on small spatial scales has an asymmetric structure, which is typically identified with a disk. A second outcome of this research is that we confirm that Herbig Ae stars are similar to T Tauri stars in displaying a line polarization effect, while depolarization is more common among Herbig Be stars. This finding had been suggested previously to indicate that Herbig Ae stars form in the same manner than T Tauri stars through magnetospheric accretion. It appears that the transition between these two differing polarization line effects occurs around the B7-B8 spectral type. This would in turn not only suggest that Herbig Ae stars accrete in a similar fashion as lower mass stars, but also that this accretion mechanism switches to a different type of accretion for Herbig Be stars. We report that the magnitude of the line effect caused by electron scattering close to the stars does not exceed 2%. Only a very weak correlation is found between the magnitude of the line effect and the spectral type or the strength of the Halpha line. This indicates that the detection of a line effect only relies on the geometry of the line-forming region and the geometry of the scattering electrons.
17 Pages, accepted for publication in MNRAS
References in corpus (10)
- A search for strong, ordered magnetic fields in Herbig Ae/Be stars
- An Unstable Truth: How Massive Stars get their Mass
- Detection of an inner gaseous component in a Herbig Be star accretion disk: Near- and mid-infrared spectro-interferometry and radiative transfer modeling of MWC 147
- Investigating the inner discs of Herbig Ae/Be stars with CO bandhead and Br Gamma emission
- On the difference between Herbig Ae and Herbig Be stars
- Spectropolarimetric Observations of Herbig Ae/Be Stars. II. Comparison of Spectropolarimetric Surveys: HAeBe, Be and Other Emission-Line Stars
- The compact H emitting regions of the Herbig Ae/Be stars HD 179218 and HD 141569 from CHARA spectro-interferometry
- Linear spectropolarimetry across the optical spectrum of Herbig Ae/Be stars
- Photoionization Models for the Inner Gaseous Disks of Herbig Be Stars: Evidence Against Magnetospheric Accretion?
- Linear line spectropolarimetry of Herbig Ae/Be stars
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- Resolving the circumstellar environment of the Galactic B[e] supergiant star MWC 137. II. Nebular kinematics and stellar variability
- Spectropolarimetry of stars across the H-R diagram
- A CCD Search for Variable Stars in the Open Cluster NGC 6611
- Identification and spectroscopic characterization of 128 new Herbig stars
- A Census of B[e] Supergiants