J/AJ/166/97            Radial velocities in W5 YSO groups           (Lim+, 2023)

The Kinematics of the Young Stellar Population in the W5 Region of the Cassiopeia OB6 Association: Implication for the Formation Process of Stellar Associations. Lim B., Hong J., Lee J., Yun H.-S., Hwang N., Park B.-G. <Astron. J., 166, 97 (2023)> =2023AJ....166...97L 2023AJ....166...97L
ADC_Keywords: Associations, stellar; Star Forming Region; YSOs; Spectra, optical; Radial velocities Keywords: Star formation ; Stellar kinematics ; Stellar associations ; Stellar dynamics ; Open star clusters Abstract: The star-forming region W5 is a major part of the Cassiopeia OB6 association. Its internal structure and kinematics may provide hints of the star formation process in this region. Here, we present a kinematic study of young stars in W5 using the Gaia data and our radial velocity data. A total 490 out of 2000 young stars are confirmed as members. Their spatial distribution shows that W5 is highly substructured. We identify a total of eight groups using the k-means clustering algorithm. There are three dense groups in the cavities of H ii bubbles, and the other five sparse groups are distributed at the edges of the bubbles. The three dense groups have almost the same age (5Myr) and show a pattern of expansion. The scale of their expansion is not large enough to account for the overall structure of W5. The three northern groups are, in fact, 3Myr younger than the dense groups, which indicates independent star formation events. Only one of these groups shows the signature of feedback- driven star formation as its members move away from the eastern dense group. The other two groups might have formed in a spontaneous way. On the other hand, the properties of two southern groups are not understood as those of a coeval population. Their origins can be explained by dynamical ejection of stars and multiple star formation. Our results suggest that the substructures in W5 formed through multiple star-forming events in a giant molecular cloud. Description: We performed multiobject spectroscopic observations of YSO candidates on 2020 September 3, October 30, and 2021 October 22, 27, and 29 using the high-resolution (R∼34000) multiobject spectrograph Hectochelle on the 6.5m telescope of the MMT observatory. All the spectra were taken with the RV31 filter, which covers the spectral range 5150-5300Å in a 2x2 binning mode. Objects: ------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------ 02 51 25.20 +60 25 08.3 W5 = C 0247+602 ------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 124 490 List of members table2.dat 75 8 Properties of individual groups -------------------------------------------------------------------------------- See also: B/mk : Catalogue of Stellar Spectral Classifications (Skiff, 2009- ) B/simbad : Simbad objects catalogue (M.Wenger 2000) I/337 : Gaia DR1 (Gaia Collaboration, 2016) I/350 : Gaia EDR3 (Gaia Collaboration, 2020) V/125 : Photometry and Spectroscopy for Luminous Stars (Reed 2005) J/AJ/128/805 : Low-mass stars in Cepheus OB2 region (Sicilia-Aguilar+ 2004) J/ApJS/160/319 : COUP; observations and source lists (Getman+, 2005) J/A+A/455/903 : ACIS-I observations of NGC 2264 (Flaccomio+, 2006) J/ApJ/639/1069 : Radial velocities in the CasOB6 association (Hillwig+, 2006) J/A+A/472/835 : JHKs and GLIMPSE photometry of RCW 120 (Zavagno+, 2007) J/ApJ/688/1142 : Star formation in W5; Spitzer observations (Koenig+, 2008) J/MNRAS/415/1202 : BVI photometry in W5E HII region (Chauhan+, 2011) J/ApJ/726/18 : Young intermediate-mass stars in W5 (Koenig+, 2011) J/A+A/539/A74 : NGC1893 Chandra X-ray catalog (Caramazza+, 2012) J/ApJ/787/107 : Spatial structure of young stellar clusters I. (Kuhn+, 2014) J/MNRAS/438/1451 : UBVIHα photometry of IC 1848 (Lim+, 2014) J/MNRAS/443/454 : UBVIHα photometry in NGC 1893 (Lim+, 2014) J/MNRAS/477/1993 : NGC 1893 stars LSR velocities (Lim+, 2018) J/ApJS/236/51 : PGCCs in lambda Orionis complex. II. Cores 850um (Yi+, 2018) J/ApJ/870/32 : Kinematics young star clusters & associations (Kuhn+, 2019) J/MNRAS/490/440 : Gaia view of Cygnus OB2 & Carina OB1 assoc (Lim+, 2019) J/ApJS/244/28 : The 3rd MSFRs Omnibus X-ray Catalog (Townsley+, 2019) J/ApJ/899/121 : 127 early type & pre-main-sequence stars in W4 (Lim+, 2020) J/MNRAS/495/663 : Gaia DR2 OB associations (Ward+, 2020) J/AJ/162/56 : Radial velocity of 240 YSO with MMT/Hectochelle (Lim+, 2021) J/ApJS/254/14 : Planck Cold Clumps lambda Orionis complex. III. (Yi+, 2021) J/AJ/163/266 : IGRINS & Gaia; star formation Monoceros OB1 &R1 (Lim+, 2022) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Seq [1/490] Sequential identifier 5- 13 F9.6 deg RAdeg [41/46] Right Ascension (J2000) 15- 23 F9.6 deg DEdeg [59/62] Declination (J2000) 25- 30 F6.4 mas plx [0.28/0.99] Gaia EDR3 parallax 32- 37 F6.4 mas e_plx [0.01/0.4] Uncertainty in plx 39- 44 F6.3 mas/yr pmRA [-2.1/1.45] Gaia EDR3 proper motion in RA 46- 50 F5.3 mas/yr e_pmRA [0.01/0.3] Uncertainty in pmRA 52- 57 F6.3 mas/yr pmDE [-2.13/1.44]? Gaia EDR3 proper motion in DE 59- 63 F5.3 mas/yr e_pmDE [0.01/0.4] Uncertainty in pmDE 65- 71 F7.3 km/s RVel [-54.1/-5.06]? Heliocentric radial velocity 73- 79 F7.3 km/s RV-LSR [-51.1/-1.99]? Radial velocity in the local standard of rest frame 81- 85 F5.3 km/s e_RVel [0.2/5]? Uncertainty in Radial Velocity 87- 93 F7.4 mag Gmag [7.81/19.2] Gaia EDR3 G-band magnitude 95-101 F7.4 mag BPmag [7.99/20.9] Gaia EDR3 BP-band magnitude 103-109 F7.4 mag RPmag [7.46/18] Gaia EDR3 RP-band magnitude 111-116 F6.4 mag BP-RP [0.48/4.32] Gaia EDR3 BP-RP color 118-122 A5 --- Remark Remarks (1) 124-124 A1 --- Group Group (Table 2) -------------------------------------------------------------------------------- Note (1): Classification of young stars ; 'E' represents O- or B-type stars obtained from the data bases of MK classification. 'H' and 'h' are Hα emission stars and Hα emission star candidates, respectively. '1', '2', and 'T' denote Class I, Class II, and YSOs with a transitional disk, respectively. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 1 A1 --- Group Group 3- 11 F9.6 deg RAdeg [41/46] Median group Right Ascension (J2000) 13- 21 F9.6 deg DEdeg [59/61] Median group Declination (J2000) 23- 28 F6.3 mas/yr pmRA [-0.62/0.21] Median group proper motion in RA 30- 35 F6.3 mas/yr pmDE [-0.64/-0.03] Median group proper motion in DE 37- 40 F4.1 km/s VT-RA [-6.1/2] Median tangential velocity in RA 42- 45 F4.1 km/s VT-DE [-6.3/-0.4] Median tangential velocity in DE 47- 51 F5.1 km/s RV-LSR [-39.2/-29.1]? Median Radial velocity in the local standard of rest frame 53- 55 F3.1 km/s sigVT-RA [2.4/6.9] Dispersion of tangential velocity along RA 57- 59 F3.1 km/s sigVT-DE [2/8.7] Dispersion of tangential velocity along DE 61- 63 F3.1 km/s sigRV-LSR [0.6/3.5]? Dispersion of RV-LSR 65- 67 I3 --- Ngrp [10/159] number of group members 69- 70 I2 --- Nrv [0/25] number of group members with RV 72- 75 F4.2 --- MST [0.62/1.73] minimum spanning tree -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 20-Mar-2024
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line