2018A&A...615A...2C


Query : 2018A&A...615A...2C

2018A&A...615A...2C - Astronomy and Astrophysics, volume 615A, 2-2 (2018/7-1)

The ionizing source of the bipolar HII region S106: A close massive binary.

COMERON F., SCHNEIDER N., DJUPVIK A.A. and SCHNUGG C.

Abstract (from CDS):


Context. S106, one of the best known bipolar HII regions, has been thoroughly studied and modeled at infrared, submillimeter, and millimeter wavelengths. This region is one of the nearest examples of the late stages of massive star formation, in which the newly formed star that ionizes it is still surrounded by vast amounts of gas and dust. However, little is known about the heavily obscured central source of this region, S106IR.
Aims. We investigate the possible binarity of the central source is investigated; this binarity is considered to be likely given the high binarity fraction among massive stars.
Methods. We have carried out visible and near-infrared photometric monitoring looking for short-term variability, and we took special interest in that related to the presence of a close binary companion to S106IR, which may produce periodic eclipses or tidal distortion of the shape of the members of the system.
Results. A periodic variability of S106IR in the J band is found with a period of 5.0-days and an amplitude of ~=0.1mag. The light curve displays a slow rise from minimum to maximum followed by a steep decrease, and can be well reproduced by a close binary system composed of two stars with different luminosities orbiting each other in an elliptical orbit of moderate eccentricity. S106IR also shows hints of short-term variability that is possibly related to accretion. We also report variability of four other stars previously classified as members of the S106 cluster, all of which are strong X-ray emitters.
Conclusions. The newly discovered close binarity of S106IR adds a new element to the modeling of the nebula and the understanding of the dynamics of the gas around the ionizing source, which suggests that the components of the binary are accreting via a circumbinary disk. Binarity also helps to explain the apparent mismatch between the spectral type of the ionizing source inferred from the nebular spectrum and its high brightness at near-infrared wavelengths.

Abstract Copyright: © ESO 2018

Journal keyword(s): stars: early-type - binaries: close - HII regions - photon-dominated region - ISM: individual objects: S106

Simbad objects: 10

goto Full paper

goto View the references in ADS

Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 NAME Orion Nebula Cluster OpC 05 35.0 -05 29           ~ 2067 1
2 [OTN2006] 335 * 20 27 19.2143925437 +37 22 35.980663428           ~ 4 0
3 2MASS J20272380+3722452 * 20 27 23.81 +37 22 45.2           ~ 4 0
4 [OTN2006] 801 * 20 27 25.2031985863 +37 23 13.568146413           ~ 4 0
5 NAME SH 2-106 IR Y*O 20 27 26.502 +37 22 42.03           ~ 157 1
6 2MASS J20272671+3721149 Y*O 20 27 26.711 +37 21 14.96           ~ 3 0
7 SH 2-106 HII 20 27 26.8 +37 22 49           ~ 416 2
8 2MASS J20272925+3722462 * 20 27 29.25 +37 22 46.3           ~ 4 0
9 2MASS J20273205+3723571 * 20 27 32.0513048560 +37 23 57.103705172           ~ 3 0
10 2MASS J20273393+3722349 Y*? 20 27 33.9289086353 +37 22 34.805393110           ~ 4 0

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2018A&A...615A...2C and select 'bookmark this link' or equivalent in the popup menu


2021.07.29-23:55:24

© Université de Strasbourg/CNRS

    • Contact