NGC7538 IRS1 - an ionized jet powered by accretion

TL;DR

This study reveals that NGC7538 IRS1 hosts a collimated ionized wind driven by accretion, with variable free-free emission and signs of heavy accretion activity, challenging simple hypercompact core models.

Contribution

It provides high-resolution analysis of the ionized wind structure and demonstrates ongoing accretion in NGC7538 IRS1 through multi-wavelength observations.

Findings

The core's flux density follows a frequency dependence with alpha ~ 0.7.

The source exhibits a steep density gradient inconsistent with a simple hypercompact core.

HCO+ observations show an inverse P Cygni profile indicating heavy accretion.

Abstract

Analysis of high spatial resolution VLA images shows that the free-free emission from NGC7538 IRS1 is dominated by a collimated ionized wind. We have re-analyzed high angular resolution VLA archive data from 6 cm to 7 mm, and measured separately the flux density from the compact bipolar core and the extended (1.5" - 3") lobes. We find that the flux density of the core is proportional to the frequency to the power of alpha, with alpha being about 0.7. The frequency dependence of the total flux density is slightly steeper with alpha = 0.8. A massive optically thick hypercompact core with a steep density gradient can explain this frequency dependence, but it cannot explain the extremely broad recombination line velocities observed in this source. Neither can it explain why the core is bipolar rather than spherical, nor the observed decrease of 4% in the flux density in less than 10 years. An ionized wind modulated by accretion is expected to vary, because the accretion flow from the surrounding cloud will vary over time. BIMA and CARMA continuum observations at 3 mm show that the free-free emission still dominates at 3 mm. HCO+ J = 1 - 0 observations combined with FCRAO single dish data show a clear inverse P Cygni profile towards IRS1. These observations confirm that IRS1 is heavily accreting with an accretion rate of about 2 times 10(-4) solar masses per year.