Photometric variability of massive young stellar objects. I

• Published in: arXiv.org
• Main Authors: Teixeira, G D C, Kumar, M S N, Smith, L, Lucas, P W, Morris, C, Borissova, J, M J P F G Monteiro, A Caratti o Garatti, C Contreras Peña, Froebrich, D, Gameiro, J F
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 13.09.2018
• Subjects: Clumps; Deposition; Infrared sources (astronomy); Infrared tracking; Outflow; Photometry; Physics - Astrophysics of Galaxies; Physics - Solar and Stellar Astrophysics; Point sources
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.1809.04882

The VVV survey has allowed for an unprecedented number of multi-epoch observations of the southern Galactic plane. In a recent paper,13 massive young stellar objects(MYSOs) have already been identified within the highly variable(\Delta Ks > 1 mag) YSO sample of another published work.This study aims to understand the general nature of variability in MYSOs.We present the first systematic study of variability in a large sample of candidate MYSOs.We examined the data for variability of the putative driving sources of all known Spitzer EGOs and bright 24 \mu m sources coinciding with the peak of 870 \mu m detected ATLASGAL clumps, a total of 718 targets. Of these, 190 point sources (139 EGOs and 51 non-EGOs) displayed variability (IQR > 0.05, \Delta Ks > 0.15 mag). Light-curves(LCs) have been sub-classified into eruptive, dipper, fader, short-term-variable and long-period variable-YSO categories.Lomb-Scargle periodogram analysis of periodic LCs was carried out. 1 - 870 \mu m spectral energy distributions of the variable sources were fitted with YSO models to obtain representative properties. 41% of the variable sources are represented by > 4Msun objects, and only 6% by > 8Msun objects.The highest-mass objects are mostly non-EGOs,deeply embedded.By placing them on the HR diagram we show that most lower mass,EGO type objects are concentrated on the putative birth-line position, while the luminous non-EGO type objects group around the ZAMS track.Some of the most luminous far infrared sources in the massive clumps and infrared quiet driving sources of EGOs have been missed out by this study owing to an uniform sample selection method.A high rate of detectable variability in EGO targets (139 out of 153 searched) implies that near-infrared variability in MYSOs is closely linked to the accretion phenomenon and outflow activity.