Star formation activity in the neighbourhood of W-R 1503-160L star in the mid-infrared bubble N46

TL;DR

This study investigates star formation around the W-R 1503-160L star in the mid-infrared bubble N46, revealing active star formation influenced by stellar winds and feedback from the Wolf-Rayet star through multi-wavelength analysis.

Contribution

It provides a detailed multi-wavelength analysis of the star formation processes and feedback effects in the environment of the mid-infrared bubble N46 containing a Wolf-Rayet star.

Findings

Identification of an expanding shell with condensations and young stellar objects.

Detection of active massive star formation in the densest condensation.

Evidence of stellar wind impact on the surrounding medium.

Abstract

In order to investigate star formation (SF) processes in extreme environments, we have carried out a multi-wavelength analysis of the mid-infrared bubble N46, which hosts a WN7 Wolf-Rayet (W-R) star. We have used 13CO line data to trace an expanding shell surrounding the W-R star containing about five condensations within the molecular cloud associated with the bubble. The W-R star is associated with a powerful stellar wind having a mechanical luminosity of ~4 x 10^37 ergs/s. A deviation of the H-band starlight mean polarization angles around the bubble has also been traced, indicating the impact of stellar wind on the surroundings. The Herschel temperature map shows a temperature range of ~18 - 24 K toward the five molecular condensations. The photometric analysis reveals that these condensations are associated with the identified clusters of young stellar objects, revealing ongoing SF process. The densest among these five condensations (peak N(H_2) ~9.2 x 10^22 cm^-2 and A_V ~ 98 mag) is associated with a 6.7 GHz methanol maser, an infrared dark cloud, and the CO outflow, tracing active massive SF within it. At least five compact radio sources (crss) are physically linked with the edges of the bubble and each of them is consistent with the radio spectral class of a B0V - B0.5V type star. The ages of the individual infrared counterparts of three crss (~1 - 2 Myr) and a typical age of WN7 W-R star (~4 Myr) indicate that the SF activities around the bubble are influenced by the feedback of the W-R star.