2010A&A...510A...5P


Query : 2010A&A...510A...5P

2010A&A...510A...5P - Astronomy and Astrophysics, volume 510, A5-5 (2010/2-1)

Three intermediate-mass young stellar objects with different properties emerging from the same natal cloud in IRAS 00117+6412.

PALAU A., SANCHEZ-MONGE A., BUSQUET G., ESTALELLA R., ZHANG Q., HO P.T.P., BELTRAN M.T. and BEUTHER H.

Abstract (from CDS):

Our main aim is to study the influence of the initial conditions of a cloud in the intermediate/high-mass star formation process. We observed with the VLA, PdBI, and SMA the centimeter and millimeter continuum, N2H+(1-0), and CO(2-1) emission associated with a dusty cloud harboring a nascent cluster with intermediate-mass protostars. At centimeter wavelengths we found a strong source, tracing a UCHII region, at the eastern edge of the dusty cloud, with a shell-like structure, and with the near-infrared counterpart falling in the center of the shell. This is presumably the most massive source of the forming cluster. About 15'' to the west of the UCHII region and well embedded in the dusty cloud, we detected a strong millimeter source, MM1, associated with centimeter and near-infrared emission. MM1 seems to be driving a prominent high-velocity CO bipolar outflow elongated in the northeast-southwest direction, and is embedded in a ridge of dense gas traced by N2H+, elongated roughly in the same direction as the outflow. We estimated that MM1 is an intermediate-mass source in the Class 0/I phase. About 15'' to the south of MM1, and still more deeply embedded in the dusty cloud, we detected a compact millimeter source, MM2, with neither centimeter nor near-infrared emission, but with water maser emission. MM2 is associated with a clump of N2H+, whose kinematics reveal a clear velocity gradient and additionally we found signposts of infall motions. MM2, being deeply embedded within the dusty cloud, with an associated water maser but no hints of CO outflow emission, is an intriguing object, presumably of intermediate mass. The UCHII region is found at the border of a dusty cloud which is currently undergoing active star formation. Two intermediate-mass protostars in the dusty cloud seem to have formed after the UCHII region and have different properties related to the outflow phenomenon. Thus, a single cloud with similar dust emission and similar dense gas column densities seems to be forming objects with different properties, suggesting that the initial conditions in the cloud are not determining all the star formation process.

Abstract Copyright:

Journal keyword(s): stars: formation - dust, extinction - HII regions - ISM: individual objects: IRAS 00117+6412 - radio continuum: ISM

VizieR on-line data: <Available at CDS (J/A+A/510/A5): maps.dat fig/*>

Nomenclature: Figs 1, 3: [PSB2010] MM1-WW (Nos MM1, MM1-S, MM1-SW, MM1-NE, MM2), [PSB2010] UCHII N=1. Paragr. 3.1: [PSB2010] JHHMMSS.ss+DDMMSS.s N=2.

Simbad objects: 25

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Number of rows : 25
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 [PSB2010] J001403.21+673226.5 Rad 00 14 03.21 +67 32 26.5           ~ 1 0
2 2MASS J00142558+6428416 NIR 00 14 25.587 +64 28 41.70           ~ 1 0
3 [PSB2010] MM1-SW mm 00 14 25.861 +64 28 42.25           ~ 1 0
4 [PSB2010] MM1-S mm 00 14 26.065 +64 28 42.26           ~ 1 0
5 2MASS J00142616+6428444 NIR 00 14 26.165 +64 28 44.44           ~ 1 1
6 [PSB2010] MM1-NE mm 00 14 26.30 +64 28 45.0           ~ 1 0
7 [PSB2010] MM2 mm 00 14 26.3 +64 28 27           ~ 14 0
8 IRAS 00117+6412 HII 00 14 26.61 +64 28 30.3           ~ 38 0
9 [PSB2010] MM1 mm 00 14 27.0 +64 28 45           ~ 13 1
10 [PSB2010] UCHII HII 00 14 28.10 +64 28 46.5           ~ 1 1
11 [SPE2008b] IRAS 00117+6412 VLA 3 HII 00 14 28.12 +64 28 46.2           ~ 2 0
12 2MASS J00142828+6428471 NIR 00 14 28.2383899447 +64 28 47.240653636           ~ 1 1
13 4C 60.01 Rad 00 14 48.7920640 +61 17 43.542069           ~ 27 1
14 [PSB2010] J001457.69+672849.6 Rad 00 14 57.69 +67 28 49.6           ~ 1 0
15 7C 0059+5808 QSO 01 02 45.76238248 +58 24 11.1366009   20.09 19.22 18.57 17.90 ~ 202 1
16 3C 48 QSO 01 37 41.2995845985 +33 09 35.079126038   16.62 16.20     ~ 2619 2
17 6C 021252+733537 BLL 02 17 30.8143057005 +73 49 32.612359669     19.0 18.97   ~ 419 1
18 4C 67.05 QSO 02 28 50.05148948 +67 21 03.0293039   19.5   18.1   ~ 239 1
19 IRAS 07427-2400 mul 07 44 51.9 -24 07 41           ~ 56 0
20 WISE J074451.99-240742.1 mul 07 44 51.997 -24 07 42.11           ~ 66 0
21 3C 286 Sy1 13 31 08.2885060664 +30 30 32.960825107   17.51 17.25     ~ 3932 2
22 EM* MWC 349 ** 20 32 45.499080 +40 39 36.74124   15.88 13.15 12.13   Bep 738 0
23 4C 06.69 QSO 21 48 05.4585565234 +06 57 38.605396596   16.85 16.47 15.06   ~ 619 1
24 6C 222905+693121 BLL 22 30 36.46970494 +69 46 28.0768954     19.6 20.11   ~ 88 1
25 3C 454.3 Bla 22 53 57.74798 +16 08 53.5611   16.57 16.10 15.22   ~ 2609 2

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2021.10.27-09:28:49

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