Study of young stellar objects and associated filamentary structures in the inner Galaxy

TL;DR

This study analyzes young stellar objects and filamentary structures in the inner Galaxy, revealing star formation sites, filament properties, and the distribution and characteristics of Class I and II sources.

Contribution

It provides a detailed catalog of YSOs, identifies major star forming filaments, and examines their properties and star formation activity in the inner Galaxy.

Findings

Identified 10 major star forming sites, 8 filamentary and 2 clusters.

Most Class I sources are aligned along filaments, indicating filamentary star formation.

Detected high-mass star formation activity in the studied regions.

Abstract

Young Stellar Objects (YSOs) in the inner Galactic region $10^0 < l < 15^0$ and $-1^0 < b < 1^0$ are studied using GLIMPSE images and GLIMPSE data catalogue. A total number of 1107 Class I and 1566 Class II sources are identified in this Galactic region. With the help of GLIMPSE 5.8 $\mu$m & 8 $\mu$m images, we have identified the presence of 10 major star forming sites in the Galactic midplane, of which 8 of them are filamentary while 2 are possible clusters of Class I $&$ II sources. The length of the identified filaments are estimated as 8'-33' ($\sim$ 9 - 56 pc). Occurrence of Hub-Filamentary System (HFS) is observed in many filamentary star forming sites. Most of the Class I sources are found to be aligned along the length of these filamentary structures, while Class II sources have a random distribution. Mass and age distribution of 425 Class I and 241 Class II sources associated with filaments & clusters are studied through their SED analysis. Most of the Class I sources detected have mass $>$ 8M$_\odot$, while Class II sources have relatively low mass regime. Class I sources have ages $\le$ 0.5 Myr, while Class II sources have ages in the range $\sim$0.1 - 3 Myr. Along with the help of high mass star forming tracers, we demonstrate that the 10 regions studied here are forming a large number of high-mass stars.