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K-band GRAVITY/VLTI interferometry of 'extreme' Herbig Be stars. The size–luminosity relation revisited
- Source :
- DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial, instname
- Publication Year :
- 2021
- Publisher :
- EDP Sciences, 2021.
-
Abstract
- (Abridged:) It has been hypothesized that the location of Herbig Ae/Be stars (HAeBes) within the empirical relation between the inner disk radius (r$_{in}$), inferred from K-band interferometry, and the stellar luminosity (L$_*$), is related to the presence of the innermost gas, the disk-to-star accretion mechanism, the dust disk properties inferred from the spectral energy distributions (SEDs), or a combination of these effects. This work aims to test whether the previously proposed hypotheses do, in fact, serve as a general explanation for the distribution of HAeBes in the size-luminosity diagram. GRAVITY/VLTI spectro-interferometric observations at $\sim $2.2 $ \mu$m have been obtained for five HBes representing two extreme cases concerning the presence of innermost gas and accretion modes. V590 Mon, PDS 281, and HD 94509 show no excess in the near-ultraviolet, Balmer region of the spectra ($\Delta$D$_B$), indicative of a negligible amount of inner gas and disk-to-star accretion, whereas DG Cir and HD 141926 show such strong $\Delta$D$_B$ values that cannot be reproduced from magnetospheric accretion, but probably come from the alternative boundary layer mechanism. Additional data for these and all HAeBes resolved through K-band interferometry have been compiled from the literature and updated using Gaia EDR3 distances, almost doubling previous samples used to analyze the size-luminosity relation. We find no general trend linking the presence of gas inside the dust destruction radius or the accretion mechanism with the location of HAeBes in the size-luminosity diagram. Underlying trends are present and must be taken into account when interpreting the size-luminosity correlation. Still, it is argued that the size-luminosity correlation is most likely to be physically relevant in spite of the previous statistical warning concerning dependencies on distance.<br />Comment: 20 pages, 17 figures. The main data reduction and analysis process ia available at https://github.com/marcosarenal/gravity-data-reduction
- Subjects :
- Protoplanetary disks
variable T Tauri, Herbig Ae/Be [Stars]
Astrophysics::High Energy Astrophysical Phenomena
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
Spectral line
Luminosity
symbols.namesake
pre-main sequence [Stars]
0103 physical sciences
Astrophysics::Solar and Stellar Astrophysics
Instrumentation and Methods for Astrophysics (astro-ph.IM)
010303 astronomy & astrophysics
Solar and Stellar Astrophysics (astro-ph.SR)
Astrophysics::Galaxy Astrophysics
Physics
010308 nuclear & particles physics
Spectral density
Balmer series
Astronomy and Astrophysics
interferometers [Instrumentation]
Radius
Astrophysics - Astrophysics of Galaxies
Accretion (astrophysics)
Interferometry
Stars
Astrophysics - Solar and Stellar Astrophysics
Space and Planetary Science
Astrophysics of Galaxies (astro-ph.GA)
Accretion disks
symbols
Astrophysics::Earth and Planetary Astrophysics
Astrophysics - Instrumentation and Methods for Astrophysics
Subjects
Details
- Language :
- English
- ISSN :
- 00046361
- Database :
- OpenAIRE
- Journal :
- DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial, instname
- Accession number :
- edsair.doi.dedup.....908fad95adfbf058024bc32d978e3943