SIMBAD references

2015ApJS..219...21Z - Astrophys. J., Suppl. Ser., 219, 21 (2015/August-0)

A deep near-infrared survey toward the Aquila molecular cloud. I. Molecular hydrogen outflows.

ZHANG M., FANG M., WANG H., SUN J., WANG M., JIANG Z. and ANATHIPINDIKA S.

Abstract (from CDS):

We have performed an unbiased, deep near-infrared survey toward the Aquila molecular cloud with a sky coverage of ∼1 deg2. We identified 45 molecular hydrogen emission-line objects (MHOs), of which only 11 were previously known. Using the Spitzer archival data, we also identified 802 young stellar objects (YSOs) in this region. Based on the morphology and the location of MHOs and YSO candidates, we associate 43 MHOs with 40 YSO candidates. The distribution of jet length shows an exponential decrease in the number of outflows with increasing length, and the molecular hydrogen outflows seem to be oriented randomly. Moreover, there is no obvious correlation between jet lengths, jet opening angles, or jet H2 1-0 S(1) luminosities and the spectral indices of the possible driving sources in this region. We also suggest that molecular hydrogen outflows in the Aquila molecular cloud are rather weak sources of turbulence, unlikely to generate the observed velocity dispersion in the region of survey.

Abstract Copyright:

Journal keyword(s): infrared: ISM - ISM: jets and outflows - shock waves - stars: formation - stars: winds, outflows

VizieR on-line data: <Available at CDS (J/ApJS/219/21): table1.dat table2.dat>

Nomenclature: Fig. 3, Table 1: [ZFW2015] NN (Nos 1-40). Fig. 3, Table 2: MHO NNNN (Nos 3259-3292) added.

Simbad objects: 59

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2021.06.21-10:32:18

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