New signposts of massive star formation in the S235A-B region

¹ INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy e-mail: fmassi@arcetri.astro.it
² Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA

Received: 5 December 2005
Accepted: 15 February 2006

Abstract

Aims.We report on new aspects of the star-forming region S235AB revealed through high-resolution observations at radio and mid-infrared wavelengths.

Methods.Using the Very Large Array, we carried out sensitive observations of S235AB in the cm continuum (6, 3.6, 1.3, and 0.7) and in the 22 GHz water maser line. These were complemented with Spitzer Space Telescope Infrared Array Camera archive data to clarify the correspondence between radio and IR sources. We made also use of newly presented data from the Medicina water maser patrol, started in 1987, to study the variability of the water masers found in the region.

Results.S235A is a classical HII region whose structure is now well resolved. To the south, no radio continuum emission is detected either from the compact molecular core or from the jet-like structure observed at 3.3 mm, suggesting emission from dust in both cases. We find two new compact radio continuum sources (VLA-1 and VLA-2) and three separate maser spots. VLA-1 coincides with one of the maser spots and with a previously identified IR source (M 1). VLA-2 lies towards S235B and represents the first radio detection from this peculiar nebula that may represent an ionized wind from a more evolved star. The two other maser spots coincide with an elongated structure previously observed within the molecular core in the C³⁴S line. This structure is perpendicular to a bipolar molecular outflow observed in HCO⁺(1-0) and may trace the associated equatorial disk. The Spitzer images reveal a red object towards the molecular core. This is the most viable candidate for the embedded source originating the outflow and maser phenomenology.

Conclusions.The picture emerging from these and previous data shows the extreme complexity of a small (≤0.5 pc) star-forming region where widely different stages of stellar evolution are present.