Near-infrared detection of H2 flows in the core of the Mon R1 association

Author:

Magakian T Yu1,Tatarnikov A M2,Movsessian T A1,Andreasyan H R1

Affiliation:

1. Byurakan Astrophysical Observatory, 0213, Aragatsotn reg., Armenia

2. M. V. Lomonosov Moscow State University, Sternberg Astronomical Institute, Universitetskij pr. 13, 119992 Moscow, Russia

Abstract

ABSTRACT We report the discovery of four new H2 jets in the Mon R1 star-forming region in images obtained with the 2.5-m telescope of the Caucasian Mountain Observatory of Sternberg Astronomical Institute (SAI), Moscow State University (MSU) through a filter centred on the H2 1–0 S(1) emission line. This discovery confirms the nature of these flows, the existence of which was previously suspected from archival Spitzer GLIMPSE360 and Wide-field Infrared Survey Explorer (WISE) survey images. Also, two infrared reflection nebulae were revealed. On Herschel Photodetecting Array Camera and Spectrometer (PACS) survey images, we found a small group of far-infrared sources, mostly unknown ones; among them are the possible exciting objects of these outflows. Spectral energy distributions of the new sources show their extremely red colour and bolometric luminosities reaching 3 L⊙ and even 10 L⊙. They are thought to be pre-main-sequence (PMS) objects in the very early evolutionary stages.

Funder

ESA

NASA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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