J/MNRAS/495/3104   Runaway and walkaway stars from the ONC   (Schoettler+, 2020)

Runaway and walkaway stars from the ONC with Gaia DR2. Schoettler C., de Bruijne J., Vaher E., Parker R.J. <Mon. Not. R. Astron. Soc., 495, 3104-3123 (2020)> =2020MNRAS.495.3104S 2020MNRAS.495.3104S (SIMBAD/NED BibCode)
ADC_Keywords: Stars, high-velocity ; Clusters, open ; Radial velocities ; Stars, ages ; Stars, masses ; Spectral types ; Optical Keywords: astrometry - stars: kinematics and dynamics - open clusters and associations: individual: Orion Nebula Cluster Abstract: Theory predicts that we should find fast, ejected (runaway) stars of all masses around dense, young star-forming regions. N-body simulations show that the number and distribution of these ejected stars could be used to constrain the initial spatial and kinematic substructure of the regions. We search for runaway and slower walkaway stars within 100pc of the Orion Nebula Cluster (ONC) using Gaia DR2 astrometry and photometry. We compare our findings to predictions for the number and velocity distributions of runaway stars from simulations that we run for 4Myr with initial conditions tailored to the ONC. In Gaia DR2, we find 31 runaway and 54 walkaway candidates based on proper motion, but not all of these are viable candidates in three dimensions. About 40 per cent are missing radial velocities, but we can trace back nine 3D runaways and 24 3D walkaways to the ONC, all of which are low/intermediate mass (<8M). Our simulations show that the number of runaways within 100pc decreases the older a region is (as they quickly travel beyond this boundary), whereas the number of walkaways increases up to 3Myr. We find fewer walkaways in Gaia DR2 than the maximum suggested from our simulations, which may be due to observational incompleteness. However, the number of Gaia DR2 runaways agrees with the number from our simulations during an age of ∼1.3-2.4Myr, allowing us to confirm existing age estimates for the ONC (and potentially other star-forming regions) using runaway stars. Description: Our target for the search for RW and WW stars is the Orion Nebula Cluster (ONC). This star-forming region is well suited for this purpose due to its proximity to the Earth (∼400pc; e.g. Grossschedl et al. 2018A&A...619A.106G 2018A&A...619A.106G, Cat. J/A+A/619/A106; Kuhn et al. 2019ApJ...870...32K 2019ApJ...870...32K, Cat. J/ApJ/870/32). We adopt the centre of the ONC as described in Kuhn et al. (2019ApJ...870...32K 2019ApJ...870...32K, Cat. J/ApJ/870/32). From this central location, we select sources within a radius of 14°, which at the distance of the ONC centre translates to a radius of ∼100pc. We apply the distances from the catalogue by Bailer-Jones et al. (2018AJ....156...58B 2018AJ....156...58B, Cat. I/347) to all sources within this radius and reduce the sample by selecting only sources with distances between 300 and 500pc, adopting a central distance of 400pc. We find 31 runaway (RW) stars and 54 walkaway (WW) stars 2D candidates with an isochronal age <4Myr after applying our criteria for candidate identification (see Tables 5 and 6). We exclude 1 RW and 1 WW candidate without RV as based on their radial distance to the ONC the RV required to get to their current position since ejection from the ONC is unreasonably large for RW or WW stars (>|500|km/s). A few 2D candidates (7 RWs and 8 WWs) with known RVs are excluded as their RVs point towards the ONC instead of away from it, so these stars cannot have originated from the ONC. Table A1 lists the excluded 2D candidates, including their reason for being excluded. Table B1 provides information on identified 2D candidates that would not be identified as RWs or WWs only by their 2D velocity, but could be when considering their RV measurements. We also find several older 3D RW/WW stars below the isochrone along the MS. These stars are possibly past 'visitors' to the ONC, having travelled through the ONC from their origin. Information about these visitors is provided in Table C1. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 110 31 RW star 2D candidates sorted by decreasing 2D velocity table6.dat 111 54 WW star 2D candidates tablea1.dat 106 17 Excluded RW and WW star 2D candidates tableb1.dat 74 4 Slow 2D candidates with multiple, varying RV measurements tablec1.dat 66 42 Past visitors to the ONC -------------------------------------------------------------------------------- See also: I/345 : Gaia DR2 (Gaia Collaboration, 2018) J/ApJ/807/27 : IN-SYNC. III. Radial velocities of IC348 stars (Cottaar+, 2015) III/252 : Pulkovo radial velocities for 35493 HIP stars (Gontcharov, 2006) J/AJ/156/84 : APOGEE-2 survey of Orion Complex. II. (Kounkel+, 2018) J/ApJ/870/32 : Kinematics in young star clusters & associations (Kuhn+, 2019) Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- GaiaDR2 Gaia DR2 source identifier 21- 25 F5.1 km/s v2Drf Rest frame 2D velocity 27- 29 F3.1 km/s e_v2Drf Error on v2Drf 31- 35 F5.1 km/s RVrf ? Rest frame radial velocity 37- 40 F4.1 km/s e_RVrf ? Error on RVrf 42- 44 A3 --- r_RVrf Reference on RVrf (1) 46- 48 A3 --- 3Dcand Indication of 3D candidate status 50- 52 F3.1 Myr Tflight ? Minimum flight time since ejection 54- 63 A10 --- f_Tflight Flag on Tflight (2) 65- 68 F4.1 Myr Ageiso Age from PARSEC isochrones (Bressan et al. 2012MNRAS.427..127B 2012MNRAS.427..127B) 70- 73 F4.1 Myr E_Ageiso Upper error on Ageiso 75- 78 F4.1 Myr e_Ageiso Lower error on Ageiso 80- 86 A7 Myr Age Age from literature 88- 90 A3 --- r_Age Reference for Age (3) 92- 98 A7 Msun Mass Mass from literature 100- 102 A3 --- r_Mass Reference for Mass (3) 104- 108 A5 --- SpType Spectral type 110 I1 --- r_SpType ? Reference for SpType (3) -------------------------------------------------------------------------------- Note (1): Reference as follows: a = Gaia DR2 (Gaia Collaboration 2018A&A...616A...1G 2018A&A...616A...1G, Cat. I/345) b = Cottaar et al. (2015ApJ...807...27C 2015ApJ...807...27C, Cat. J/ApJ/807/27) d = Multiple and varying RV measurements, possibly indicating a binary system Note (2): Reference as follows: c = Age estimate is smaller than the flight time Note (3): References as follows: 1 = van Altena et al. (1988AJ.....95.1744V 1988AJ.....95.1744V) 2 = Hillenbrand (1997AJ....113.1733H 1997AJ....113.1733H, Cat. J/AJ/113/1733) 3 = Houk & Swift (1999MSS...C05....0H 1999MSS...C05....0H, Cat. III/214) 4 = Rebull et al. (2000AJ....119.3026R 2000AJ....119.3026R, Cat. J/AJ/119/3026) 5 = Da Rio et al. (2016ApJ...818...59D 2016ApJ...818...59D, Cat. J/ApJ/818/59) 6 = Nesterov et al. (1995A&AS..110..367N 1995A&AS..110..367N, Cat. III/182) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- GaiaDR2 Gaia DR2 source identifier 21- 24 F4.1 km/s v2Drf Rest frame 2D velocity 26- 28 F3.1 km/s e_v2Drf Error on v2Drf 30- 34 F5.1 km/s RVrf ? Rest frame radial velocity 36- 39 F4.1 km/s e_RVrf ? Error on RVrf 41 A1 --- r_RVrf Reference on RVrf (1) 43- 45 A3 --- 3Dcand Indication of 3D candidate status 47- 49 F3.1 Myr Tflight ? Minimum flight time since ejection 51- 60 A10 --- f_Tflight Flag on Tflight (2) 62 A1 --- u_Ageiso [~] Uncertainty flag on Ageiso 64- 67 F4.1 Myr Ageiso Age from PARSEC isochrones (Bressan et al. 2012MNRAS.427..127B 2012MNRAS.427..127B) 69- 72 F4.1 Myr E_Ageiso ? Upper error on Ageiso 74- 77 F4.1 Myr e_Ageiso ? Lower error on Ageiso 79- 85 A7 Myr Age Age from literature 87- 90 A4 --- r_Age Reference for Age (3) 92- 98 A7 Msun Mass Mass from literature 100- 103 A4 --- r_Mass Reference for Mass (3) 105- 108 A4 --- SpType Spectral type 110- 111 I2 --- r_SpType ? Reference for SpType (3) -------------------------------------------------------------------------------- Note (1): Reference as follows: a = Gaia DR2 (Gaia Collaboration 2018A&A...616A...1G 2018A&A...616A...1G, Cat. I/345) b = Cottaar et al. (2015ApJ...807...27C 2015ApJ...807...27C, Cat. J/ApJ/807/27) c = Gontcharov (2006AstL...32..759G 2006AstL...32..759G, Cat III/252) d = Kounkel et al. (2018AJ....156...84K 2018AJ....156...84K, Cat. J/AJ/156/84) Note (2): Flag as follows: e = Age estimate is smaller than the flight time Note (3): References as follows: 1 = van Altena et al. (1988AJ.....95.1744V 1988AJ.....95.1744V) 2 = Hillenbrand (1997AJ....113.1733H 1997AJ....113.1733H, Cat. J/AJ/113/1733) 3 = Houk & Swift (1999MSS...C05....0H 1999MSS...C05....0H, Cat. III/214) 4 = Rebull et al. (2000AJ....119.3026R 2000AJ....119.3026R, Cat. J/AJ/119/3026) 5 = Da Rio et al. (2010ApJ...722.1092D 2010ApJ...722.1092D, Cat. J/ApJ/722/1092) 6 = Tetzlaff et al. (2011MNRAS.410..190T 2011MNRAS.410..190T, Cat. J/MNRAS/410/190) 7 = Da Rio et al. (2012ApJ...748...14D 2012ApJ...748...14D, Cat. J/ApJ/748/14) 8 = Hsu et al. (2012ApJ...752...59H 2012ApJ...752...59H, Cat. J/ApJ/752/59) 9 = Hsu et al. (2013ApJ...764..114H 2013ApJ...764..114H, Cat. J/ApJ/764/114) 10 = Da Rio et al. (2016ApJ...818...59D 2016ApJ...818...59D, Cat. J/ApJ/818/59) 11 = Sota et al. (2011ApJS..193...24S 2011ApJS..193...24S, Cat. III/274) 12 = Hohle, Neuhauser & Schutz (2010AN....331..349H 2010AN....331..349H, Cat. J/AN/331/349) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 21 A21 --- Sample Star candidate sample (RW or WW) 23- 41 I19 --- GaiaDR2 Gaia DR2 source identifier 43- 46 F4.1 km/s v2Drf Rest frame 2D velocity 48- 50 F3.1 km/s e_v2Drf Error on v2Drf 52- 56 F5.1 km/s RVrf ? Rest frame radial velocity 58- 60 F3.1 km/s e_RVrf ? Error on RVrf 62 A1 --- r_RVrf Reference on RVrf (1) 64- 84 A21 --- Exc Exclusion reason 86- 90 F5.1 Myr Age ? Age from literature 92 I1 --- r_Age ? Reference for Age (2) 94- 96 F3.1 Msun Mass ? Mass from literature 98 I1 --- r_Mass ? Reference for Mass (2) 100- 104 A5 --- SpType Spectral type 106 I1 --- r_SpType ? Reference for SpType (2) -------------------------------------------------------------------------------- Note (1): Reference as follows: a = Gaia DR2 (Gaia Collaboration 2018A&A...616A...1G 2018A&A...616A...1G, Cat. I/345) b = Cottaar et al. (2015ApJ...807...27C 2015ApJ...807...27C, Cat. J/ApJ/807/27) c = Gontcharov (2006AstL...32..759G 2006AstL...32..759G, Cat III/252) Note (2): Reference as follows: 1 = Da Rio et al. (2016ApJ...818...59D 2016ApJ...818...59D, Cat. J/ApJ/818/59) 2 = Houk & Swift (1999MSS...C05....0H 1999MSS...C05....0H, Cat. III/214) 3 = Nesterov et al. (1995A&AS..110..367N 1995A&AS..110..367N, Cat. III/182) 4 = Houk & Smith-Moore (1988mcts.book.....H 1988mcts.book.....H) 5 = Tetzlaff et al. (2011MNRAS.410..190T 2011MNRAS.410..190T, Cat. J/MNRAS/410/190) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- GaiaDR2 Gaia DR2 source identifier 21- 23 F3.1 km/s v2Drf Rest frame 2D velocity 25- 27 F3.1 km/s e_v2Drf Error on v2Drf 29- 31 A3 --- refRV References for the rest frame radial velocity (1) 33 A1 --- 3Dcand Indication of 3D candidate status 35- 44 A10 --- fTflight Remark on flight time 46- 48 F3.1 Myr Ageiso Age from PARSEC isochrones (Bressan et al. 2012MNRAS.427..127B 2012MNRAS.427..127B) 50- 53 F4.1 Myr E_Ageiso Upper error on Ageiso 55- 57 F3.1 Myr e_Ageiso Lower error on Ageiso 59- 61 F3.1 Myr Age Age from literature 63 I1 --- r_Age Reference for Age (2) 65- 67 F3.1 Msun Mass Mass from literature 69 I1 --- r_Mass Reference for Mass (2) 71- 72 A2 --- SpType Spectral type 74 I1 --- r_SpType ? Reference for SpType (2) -------------------------------------------------------------------------------- Note (1): Reference as follows: a = Gaia DR2 (Gaia Collaboration 2018A&A...616A...1G 2018A&A...616A...1G, Cat. I/345) b = Cottaar et al. (2015ApJ...807...27C 2015ApJ...807...27C, Cat. J/ApJ/807/27) c = Kounkel et al. (2018AJ....156...84K 2018AJ....156...84K, Cat. J/AJ/156/84) Note (2): Reference as follows: 1 = Hillenbrand (1997AJ....113.1733H 1997AJ....113.1733H, Cat. J/AJ/113/1733) 2 = Da Rio et al. (2016ApJ...818...59D 2016ApJ...818...59D, Cat. J/ApJ/818/59) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablec1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 A2 --- Sample [RW/WW] Velocity type of the visitor 4- 22 I19 --- GaiaDR2 Gaia DR2 source identifier 24- 27 F4.1 km/s v2Drf Rest frame 2D velocity 29- 31 F3.1 km/s e_v2Drf Error on v2Drf 33- 37 F5.1 km/s RVrf Rest frame radial velocity 39- 42 F4.1 km/s e_RVrf Error on RVrf 44 A1 --- r_RVrf [a] Reference for RVrf (1) 46 A1 --- u_Ageiso [~] Uncertainty flag on Ageiso 48- 53 A6 Myr Ageiso Age from PARSEC isochrones (Bressan et al. 2012MNRAS.427..127B 2012MNRAS.427..127B) 55- 58 F4.1 Myr Age ? Age from literature 60 I1 --- r_Age ? Reference for Age (2) 62- 64 F3.1 Msun Mass ? Mass from literature 66 I1 --- r_Mass ? Reference for Mass (2) -------------------------------------------------------------------------------- Note (1): Reference as follows: a = Gaia DR2 (Gaia Collaboration 2018A&A...616A...1G 2018A&A...616A...1G, Cat. I/345) Note (2): Reference as follows: 1 = Da Rio et al. (2016ApJ...818...59D 2016ApJ...818...59D, Cat. J/ApJ/818/59) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Ana Fiallos [CDS] 19-Jun-2023
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