J/A+A/668/A13       Open clusters housing classical Cepheids       (Hao+, 2022)

Open clusters housing classical Cepheids in Gaia DR3. Hao C.J., Xu Y., Wu Z.Y., Lin Z.H., Bian S.B., Li Y.J., Liu D.J. <Astron. Astrophys. 668, A13 (2022)> =2022A&A...668A..13H 2022A&A...668A..13H (SIMBAD/NED BibCode)
ADC_Keywords: Milky Way ; Clusters, open ; Stars, variable ; Optical ; Parallaxes, trigonometric ; Proper motions ; Radial velocities Keywords: Galaxy: stellar content - open clusters and associations: general - stars: variables: Cepheids - methods: data analysis Abstract: The latest Gaia Data Release 3 provides an opportunity to expand the census of Galactic open clusters harboring classical Cepheid variables, thereby providing a means to bolster the cosmic distance scale. A comprehensive analysis yielded a total of 50 classical Cepheids associated with 45 open clusters, of which 39 open cluster and classical Cepheid pairs are considered believable, and the remaining 11 pairs should be improbable but worth following up. Indeed, two clusters identified previously by Hao et al. (2022A&A...660A...4H 2022A&A...660A...4H, Cat. J/A+A/660/A4) possibly host classical Cepheids (OC-0125/V1788 Cyg and OC-0675/OGLE-BLG-CEP-114). In addition, 38 new open cluster candidates were also identified within the Galactic disc. Description: Combining the high-precision data provided by Gaia DR3 and known classical Cepheids with our previously practiced clustering search method, we conducted a search for OCs containing classical Cepheids. We identified 50 classical Cepheids associated with 45 OCs in 5D astrometric space. After investigating the ages of the OCs and the periods of the Cepheids, we found 39 OC-Cepheid pairs to be probable, and a remaining 11 Cepheids to be improbable and possibly unrelated to OCs but worthy of follow-up investigation. For all of these OCz-Cepheid pairs, we provide their astrometric and astrophysical parameters. In addition to re-detecting 635 known OCs in the literature, we also propose 38 newly found OC candidates within the Galactic disk based on a detailed inspection of the multidimensional distributions of their member stars. For each of these new OC candidates, we present its mean astrometric values and radial velocity when available, together with estimations of age, line-of-sight extinction, and distance modulus. The new OCs are generally located at greater distances from the Sun, which can help to improve the completeness of the Galactic OC census. Table 1 contains parameters of the OC-Cepheid pairs identified in this work. Table 2 contains parameters of the proposed newly found OCs. Table 3 contains the member stars of open clusters housing classical Cepheids. Table 4 contains the member stars found for the new open clusters reported in the work. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 190 50 Parameters for open clusters and Cepheid pairs table2.dat 143 38 Mean parameters for the new open clusters table3.dat 174 7449 Members for open clusters housing Cepheids table4.dat 167 1883 Members for the new open clusters -------------------------------------------------------------------------------- See also: I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) J/A+A/660/A4 : Gaia EDR3 new Galactic open clusters (Hao+, 2022) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 23 A23 --- Name Cepheid name 25- 30 F6.2 deg RAdeg Cepheid Right Ascension (ICRS) at Ep=2016.0 32- 35 F4.2 deg e_RAdeg Cepheid Right Ascension error 37- 42 F6.2 deg DEdeg Cepheid Declination (ICRS) at Ep=2016.0 44- 47 F4.2 deg e_DEdeg Cepheid Declination error 49- 52 F4.2 [d] logPer Logarithm of the Cepheid pulsation period 54- 66 A13 --- Cluster Cluster name 68- 73 F6.2 deg RAodeg Cluster Right Ascension (ICRS) at Ep=2016.0 75- 78 F4.2 deg s_RAodeg Cluster Right Ascension standard deviation 80- 85 F6.2 deg DEodeg Cluster Declination mean (ICRS) at Ep=2016.0 87- 90 F4.2 deg s_DEodeg Cluster Declination standard deviation 92- 95 F4.1 arcmin sdeg Angular distance between Cluster and Cepheid 97-100 F4.1 deg adeg Cluster apparent angular size 102-106 F5.2 mas/yr pmRA Cepheid Proper motion in right ascension, pmRA*cosDE 108-111 F4.2 mas/yr e_pmRA Cepheid pmRA error 113-117 F5.2 mas/yr pmDE Cepheid Proper motion in declination 119-122 F4.2 mas/yr e_pmDE Cepheid pmDE error 124-128 F5.2 mas/yr pmRAoc Cluster Proper motion in right ascension mean, pmRA*cosDE 130-133 F4.2 mas/yr s_pmRAoc Cluster Proper motion in right ascension standard deviation 135-139 F5.2 mas/yr pmDEoc Cluster Proper motion in declination mean 141-144 F4.2 mas/yr s_pmDEoc Cluster Proper motion in declination standard deviation 146-149 F4.2 mas plx Cepheid Parallax 151-154 F4.2 mas e_plx Cepheid parallax error 156-159 F4.2 mas plxoc Cluster Parallax mean 161-164 F4.2 mas s_plxoc Cluster Parallax standard deviation 166-169 F4.2 [yr] logAge Logarithm of the Cepheid age 171-174 A4 [yr] e_logAge ?=- Error of the Cepheid age 176-179 F4.2 [yr] logAgeoc Logarithm of the cluster age 181-184 F4.2 [yr] e_logAgeoc Error of the cluster age 186-188 I3 --- Nmemb Number of cluster members 190 A1 --- Class [ABC] Class of OC-Cepheid pairs -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 17 A17 --- Cluster Cluster name (OC-NNNN) 19- 24 F6.2 deg RAdeg Right Ascension (ICRS) at Ep=2016.0 26- 29 F4.2 deg s_RAdeg Right Ascension standard deviation 31- 36 F6.2 deg DEdeg Declination mean (ICRS) at Ep=2016.0 38- 41 F4.2 deg s_DEdeg Declination standard deviation 43- 48 F6.2 deg GLON Galactic longitude mean 50- 53 F4.2 deg s_GLON Galactic longitude standard deviation 55- 59 F5.2 deg GLAT Galactic latitude mean 61- 64 F4.2 deg s_GLAT Galactic latitude standard deviation 66- 69 F4.2 deg adeg Apparent angular size 71- 74 F4.2 mas plx Parallax mean 76- 79 F4.2 mas s_plx Parallax standard deviation 81- 85 F5.2 mas/yr pmRA Proper motion in right ascension mean, pmRA*cosDE 87- 90 F4.2 mas/yr s_pmRA Proper motion in right ascension standard deviation 92- 96 F5.2 mas/yr pmDE Proper motion in declination mean 98-101 F4.2 mas/yr s_pmDE Proper motion in declination standard deviation 103-106 F4.2 [yr] logAge Logarithm of the cluster age 108-111 F4.2 [yr] e_logAge Error of the cluster age 113-116 F4.2 mag AG Line-of-sight extinction 118-122 F5.2 mag DMNN Distance modulus of the cluster 124-129 A6 km/s RV ?=- Radial velocity mean 131-136 A6 km/s s_RV ?=- Radial velocity weighted standard deviation 138-140 I3 --- Nmemb Number of cluster members 142-143 I2 --- NmembRV Number of cluster members with Gaia radial velocity measurements -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- GaiaDR3 Gaia DR3 source_id 21- 30 F10.6 deg RAdeg Right Ascension (ICRS) at Ep=2016.0 32- 41 F10.6 deg DEdeg Declination (ICRS) at Ep=2016.0 43- 52 F10.6 deg GLON Galactic longitude 54- 62 F9.6 deg GLAT Galactic latitude 64- 71 F8.6 mas plx Parallax 73- 80 F8.6 mas e_plx Parallax error 82- 90 F9.6 mas/yr pmRA Proper motion in right ascension, pmRA*cosDE 92- 99 F8.6 mas/yr e_pmRA pmRA error 101-109 F9.6 mas/yr pmDE Proper motion in declination 111-118 F8.6 mas/yr e_pmDE pmDE error 120-130 F11.6 km/s RV ? Radial velocity 132-140 F9.6 km/s e_RV ? Radial velocity error 142-150 F9.6 mag Gmag Gaia G magnitude 152-160 F9.6 mag BP-RP ? Gaia BP-RP colour 162-174 A13 --- Cluster Cluster name -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- GaiaDR3 Gaia DR3 source_id 21- 30 F10.6 deg RAdeg Right Ascension (ICRS) at Ep=2016.0 32- 41 F10.6 deg DEdeg Declination (ICRS) at Ep=2016.0 43- 52 F10.6 deg GLON Galactic longitude 54- 62 F9.6 deg GLAT Galactic latitude 64- 71 F8.6 mas plx Parallax 73- 80 F8.6 mas e_plx Parallax error 82- 90 F9.6 mas/yr pmRA Proper motion in right ascension, pmRA*cosDE 92- 99 F8.6 mas/yr e_pmRA pmRA error 101-109 F9.6 mas/yr pmDE Proper motion in declination 111-118 F8.6 mas/yr e_pmDE pmDE error 120-130 F11.6 km/s RV ? Radial velocity 132-140 F9.6 km/s e_RV ? Radial velocity error 142-150 F9.6 mag Gmag Gaia G magnitude 152-159 F8.6 mag BP-RP ? Gaia BP-RP colour 161-167 A7 --- Cluster Cluster name (OC-NNNN) -------------------------------------------------------------------------------- Acknowledgements: Ye Xu, xuye(at)pmo.ac.cn Choajie Hao, cjhao(at)pmo.ac.cn
(End) Patricia Vannier [CDS] 26-Sep-2022
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