New Herbig-Haro Objects associated with Embedded Sources

Fuente: arXiv
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Autori principali: Movsessian, T. A., Magakian, T. Yu., Reipurth, B., Andreasyan, H. R.
Natura: Preprint
Pubblicazione: 2024
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author Movsessian, T. A.
Magakian, T. Yu.
Reipurth, B.
Andreasyan, H. R.
author_facet Movsessian, T. A.
Magakian, T. Yu.
Reipurth, B.
Andreasyan, H. R.
contents We continue to present the results of the Byurakan Narrow Band Imaging Survey (BNBIS). The main goal of this survey is to search for Herbig-Haro (HH) objects and jets in Galactic dark clouds. In this work we present the results of the search in the vicinity of infrared sources that are bright in the WISE survey and embedded in the dark clouds. The survey is performed with the 1 m Schmidt telescope of Byurakan Observatory, lately equipped with a new CCD detector, which allows to obtain one square degree images of the sky in various filters. Narrow-band filters were used to obtain Halpha and [S II] images, and a medium-width filter was used for the continuum imaging. New HH flows and knots were found near six embedded IR sources, which constitutes a significant proportion of the objects observed. At least two of the newly found HH flows (HH 1226 and HH 1227) lie in isolated dark clouds, thus pointing to active star formation in these regions. Other flows are also located in detached and dense globules or filaments. The length of the HH 1228 flow is about 1 pc; it has also a molecular hydrogen counterpart of the same extension. Coordinates, charts, detailed descriptions and distance estimates are provided. The lower limits of bolometric luminosities of the source stars are typical for low-mass young stellar objects.
format Preprint
id arxiv_https___arxiv_org_abs_2404_02891
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle New Herbig-Haro Objects associated with Embedded Sources
Movsessian, T. A.
Magakian, T. Yu.
Reipurth, B.
Andreasyan, H. R.
Solar and Stellar Astrophysics
Astrophysics of Galaxies
We continue to present the results of the Byurakan Narrow Band Imaging Survey (BNBIS). The main goal of this survey is to search for Herbig-Haro (HH) objects and jets in Galactic dark clouds. In this work we present the results of the search in the vicinity of infrared sources that are bright in the WISE survey and embedded in the dark clouds. The survey is performed with the 1 m Schmidt telescope of Byurakan Observatory, lately equipped with a new CCD detector, which allows to obtain one square degree images of the sky in various filters. Narrow-band filters were used to obtain Halpha and [S II] images, and a medium-width filter was used for the continuum imaging. New HH flows and knots were found near six embedded IR sources, which constitutes a significant proportion of the objects observed. At least two of the newly found HH flows (HH 1226 and HH 1227) lie in isolated dark clouds, thus pointing to active star formation in these regions. Other flows are also located in detached and dense globules or filaments. The length of the HH 1228 flow is about 1 pc; it has also a molecular hydrogen counterpart of the same extension. Coordinates, charts, detailed descriptions and distance estimates are provided. The lower limits of bolometric luminosities of the source stars are typical for low-mass young stellar objects.
title New Herbig-Haro Objects associated with Embedded Sources
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2404.02891