Disentangling the two sub-populations of early Herbig Be stars using VLT/X-Shooter spectra

Abstract

Early Herbig Be (HBe) stars are massive, young stars accreting through the Boundary Layer mechanism. However, given the rapid ($<$ 2 Myr) evolution of early Herbig stars to the main-sequence phase, studying the evolution of the circumstellar medium around these stars can be a cumbersome exercise. In this work, we study the sample of early (B0-B5) HBe stars using the correlation between H$\alpha$ emission strength and near--infrared excess, complemented by the analysis of various emission features in the X-Shooter spectra. We segregate the sample of 37 early HBe stars based on the median values of H$\alpha$ equivalent width (EW) and near--infrared index (n(J$-$H)) distributions. The stars with |H$\alpha$ EW| $>$ 50 Å and n(J$-$H) $>$ -2 are classified as intense HBe stars and stars with |H$\alpha$ EW| $<$ 50 Å and n(J$-$H) $<$ -2 as weak HBe stars. Using the VLT/X--Shooter spectra of five intense and eight weak HBe stars, we visually checked for the differences in intensity and profiles of various H{\sc I} and metallic emission lines commonly observed in Herbig stars. We propose that the intense HBe stars possess an inner disk close to the star (as apparent from the high near-infrared excess) and an active circumstellar environment (as seen from high H$\alpha$ EW value and presence of emission lines belonging to Fe{\sc II}, Ca{\sc II}, O{\sc I} and [O{\sc I}]). However, for weak HBe stars, the inner disk has cleared, and the circumstellar environment appears more evolved than for intense HBe stars. Furthermore, we compiled a sample of $\sim$58,000 emission-line stars published in \textit{Gaia DR3} to identify more intense HBe candidates. Further spectroscopic studies of these candidates will help us to understand the evolution of the inner ($\sim$a few au) disk in early HBe stars.

arXiv commentAccepted for publication in Astronomy & Astrophysics journal. 14 pages, 7 figures and 2 tables

References in corpus (44)

• The Gaia mission
• Gaia Data Release 3: Summary of the content and survey properties
• MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
• Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3
• MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones
• The Optical to Mid-Infrared Extinction Law Based on the APOGEE, Gaia DR2, Pan-STARRS1, SDSS, APASS, 2MASS and WISE Surveys
• A spectroscopic survey of Herbig Ae/Be stars with X-Shooter I: Stellar parameters and accretion rates
• On the formation of H-alpha line emission around classical T Tauri stars
• Can we predict the global magnetic topology of a pre-main sequence star from its position in the Hertzsprung-Russell diagram?
• Gaia DR2 study of Herbig Ae/Be stars
• The Second Data Release of the INT Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS DR2)
• Gaia Data Release 3: Apsis II -- Stellar Parameters
• Evolution of emission line activity in intermediate mass young stars
• Accretion rates and accretion tracers of Herbig Ae/Be stars
• The accretion rates and mechanisms of Herbig Ae/Be stars
• 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
• Homogeneous study of Herbig Ae/Be stars from spectral energy distributions and Gaia EDR3
• Catalogue of new Herbig Ae/Be and classical Be stars. A machine learning approach to Gaia DR2
• The magnetic fields of intermediate-mass T Tauri stars : I. Magnetic detections and fundamental stellar parameters
• The pre- versus post-main sequence evolutionary phase of B[e] stars: Constraints from 13CO band emission
• Optical spectroscopic variability of Herbig Ae/Be stars
• Diagnosing Mass Flows Around Herbig Ae/Be Stars Using the He I 10830 Line
• Kinematical structure of the circumstellar environments of galactic B[e]-type stars
• Scanning disk rings and winds in CO at 0.01-10 au: a high-resolution $M$-band spectroscopy survey with IRTF-iSHELL
• On the mass accretion rate and infrared excess in Herbig Ae/Be Stars
• A family portrait of disk inner rims around Herbig Ae/Be stars: Hunting for warps, rings, self shadowing, and misalignments in the inner astronomical units
• The 2008 Outburst in the Young Stellar System Z CMa: The First Detection of Twin Jets
• Optical Mass Flow Diagnostics in Herbig Ae/Be Stars
• New Herbig Ae/Be stars confirmed via high-resolution optical spectroscopy
• On the nature of the Herbig B[e] star binary system V921 Scorpii: Geometry and kinematics of the circumprimary disk on sub-AU scales
• Herbig Stars: A Quarter Century of Progress
• Observing the linked depletion of dust and CO gas at 0.1-10 au in disks of intermediate-mass stars
• MWC 297: a young high-mass star rotating at critical velocity
• On the Mass Accretion Rates of Herbig Ae/Be Stars. Magnetospheric Accretion or Boundary Layer?
• On the nature of the Herbig B[e] star binary system V921 Scorpii: Discovery of a close companion and relation to the large-scale bipolar nebula
• Tracing Accretion onto Herbig Ae/Be Stars Using the Brγ Line
• Excitation mechanism of OI lines in Herbig Ae/Be stars
• HD 85567: A Herbig B[e] star or an interacting B[e] binary
• An Inner Gaseous Disk around the Herbig Be Star MWC 147
• Spectroscopy and Linear Spectropolarimetry of the early Herbig Be Stars PDS 27 and PDS 37
• Photoionization Models for the Inner Gaseous Disks of Herbig Be Stars: Evidence Against Magnetospheric Accretion?
• K-band GRAVITY/VLTI interferometry of "extreme" Herbig Be stars. The size-luminosity relation revisited
• Emission line star catalogues post-Gaia DR3: A validation of Gaia DR3 data using LAMOST OBA emission catalogue
• Resolving the circumstellar environment of the Galactic B[e] supergiant star MWC 137. II. Nebular kinematics and stellar variability