2019ApJ...886..119C


Query : 2019ApJ...886..119C

2019ApJ...886..119C - Astrophys. J., 886, 119-119 (2019/December-1)

Droplets. II. Internal velocity structures and potential rotational motions in pressure-dominated coherent structures.

CHEN H.H.-H., PINEDA J.E., OFFNER S.S.R., GOODMAN A.A., BURKERT A., FRIESEN R.K., ROSOLOWSKY E., SCIBELLI S. and SHIRLEY Y.

Abstract (from CDS):

We present an analysis of the internal velocity structures of the newly identified sub-0.1 pc coherent structures, droplets, in L1688 and B18. By fitting 2D linear velocity fields to the observed maps of velocity centroids, we determine the magnitudes of linear velocity gradients and examine the potential rotational motions that could lead to the observed velocity gradients. The results show that the droplets follow the same power-law relation between the velocity gradient and size found for larger-scale dense cores. Assuming that rotational motion giving rise to the observed velocity gradient in each core is a solid-body rotation of a rotating body with a uniform density, we derive the "net rotational motions" of the droplets. We find a ratio between rotational and gravitational energies, β, of ∼0.046 for the droplets, and when including both droplets and larger-scale dense cores, we find β ∼ 0.039. We then examine the alignment between the velocity gradient and the major axis of each droplet, using methods adapted from the histogram of relative orientations introduced by Soler et al. We find no definitive correlation between the directions of velocity gradients and the elongations of the cores. Lastly, we discuss physical processes other than rotation that may give rise to the observed velocity field.

Abstract Copyright: © 2019. The American Astronomical Society.

Journal keyword(s): Interstellar dynamics - Molecular clouds - Star formation - Star forming regions - Radio astronomy

Simbad objects: 27

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Number of rows : 27
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 1333 OpC 03 29 09.2 +31 20 59           ~ 1575 1
2 [EYG2006] Bolo 70 cor 03 32 44.0 +31 00 00           ~ 10 0
3 [EYG2006] Bolo 82 cor 03 33 25.1 +31 05 35           ~ 9 0
4 JCMTSE J033327.1+310701 cor 03 33 27.29 +31 07 10.2           ~ 55 0
5 LDN 1471 DNe 03 48.0 +32 54           ~ 349 0
6 [CPG2019] B18-d2 cor 04 29 24.13 +24 34 42.2           ~ 2 0
7 [CPG2019] B18-d3 cor 04 30 05.71 +24 25 40.6           ~ 2 0
8 [CPG2019] B18-d4 cor 04 31 54.48 +24 32 28.2           ~ 2 0
9 NAME Kutner's Cloud MoC 04 32 44.6 +24 23 13           ~ 283 0
10 [CPG2019] B18-d6 cor 04 35 36.32 +24 09 00.7           ~ 2 0
11 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
12 NAME Ori A MoC 05 38 -07.1           ~ 3187 0
13 [CPG2019] L1688-c1W cor 16 26 45.22 -24 33 30.5           ~ 2 0
14 [CPG2019] L1688-d1 cor 16 26 47.07 -24 33 08.3           ~ 2 0
15 [CPG2019] L1688-c1E cor 16 26 49.36 -24 32 39.0           ~ 2 0
16 [CPG2019] L1688-c2 cor 16 26 56.89 -24 30 18.7           ~ 2 0
17 [CPG2019] L1688-c3 cor 16 26 59.22 -24 33 05.9           ~ 3 0
18 [CPG2019] L1688-d4 cor 16 26 59.59 -24 34 28.8           ~ 2 0
19 [CPG2019] L1688-d5 cor 16 27 04.96 -24 39 17.6           ~ 3 0
20 [CPG2019] L1688-c4 cor 16 27 22.28 -24 24 52.2           ~ 2 0
21 [CPG2019] L1688-d6 cor 16 27 25.50 -24 41 06.2           ~ 2 0
22 [CPG2019] L1688-d7 cor 16 27 37.27 -24 42 50.2           ~ 2 0
23 [CPG2019] L1688-d8 cor 16 27 46.44 -24 44 45.4           ~ 2 0
24 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3969 1
25 [CPG2019] L1688-d10 cor 16 28 22.12 -24 36 16.8           ~ 4 0
26 [CPG2019] L1688-d11 cor 16 28 31.53 -24 18 36.1           ~ 2 0
27 [CPG2019] L1688-d12 cor 16 28 59.99 -24 20 45.2           ~ 4 0

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