A New Revision of the Stellar Content and Physical Properties of the Young Open Cluster vdB 130 in the Region of the Stellar Association CygOB1 Based on Gaia DR3 Data
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作者:
Rastorguev, A. S.
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Moscow MV Lomonosov State Univ, Moscow 119234, Russia
Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119234, RussiaMoscow MV Lomonosov State Univ, Moscow 119234, Russia
Rastorguev, A. S.
[1
,2
]
Zabolotskikh, M. V.
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Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119234, RussiaMoscow MV Lomonosov State Univ, Moscow 119234, Russia
Zabolotskikh, M. V.
[2
]
Sitnik, T. G.
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Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119234, RussiaMoscow MV Lomonosov State Univ, Moscow 119234, Russia
Sitnik, T. G.
[2
]
Wiebe, D. S.
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Russian Acad Sci, Inst Astron, Moscow 119017, RussiaMoscow MV Lomonosov State Univ, Moscow 119234, Russia
Wiebe, D. S.
[3
]
Tatarnikov, A. M.
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Moscow MV Lomonosov State Univ, Moscow 119234, Russia
Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119234, RussiaMoscow MV Lomonosov State Univ, Moscow 119234, Russia
Tatarnikov, A. M.
[1
,2
]
Tatarnikova, A. A.
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Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119234, RussiaMoscow MV Lomonosov State Univ, Moscow 119234, Russia
Tatarnikova, A. A.
[2
]
Topchieva, A. P.
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Russian Acad Sci, Inst Astron, Moscow 119017, RussiaMoscow MV Lomonosov State Univ, Moscow 119234, Russia
Topchieva, A. P.
[3
]
Tatarnikov, A. A.
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Moscow MV Lomonosov State Univ, Moscow 119234, Russia
Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119234, RussiaMoscow MV Lomonosov State Univ, Moscow 119234, Russia
Tatarnikov, A. A.
[1
,2
]
机构:
[1] Moscow MV Lomonosov State Univ, Moscow 119234, Russia
[2] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119234, Russia
[3] Russian Acad Sci, Inst Astron, Moscow 119017, Russia
stars: formation-stars: pre-main-sequence;
protostars-open clusters and associations:general-open clusters and associations: individual: vdB130;
STAR-FORMING REGIONS;
OB ASSOCIATIONS;
EXTINCTION;
PERIPHERY;
MOTIONS;
GALAXY;
D O I:
10.1134/S1990341323020050
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Based onGaiaDR3 data, a new revision of the stellar content is performedwithin the 20'-radius field centered on the young open cluster vdB 130, which is a part of the CygOB1 stellar association. A total of 97 stars and 39 protostars of luminosity classes I/II/III are identified that have proper-motion based clustermembership probabilitiesP > 0.98. The total number of possible cluster memberswithmembership probabilitiesP > 0.50 is equal to about 300, and the cluster age estimated by fitting theoretical isochrones does not exceed 10 Myr. The trigonometric-parallax based cluster distance is D approximate to 1670 +/- 60 pc, and the cluster color excess, E(BP - RP) approximate to 0(m).85 +/- 0(m).02 with evidence for strong differential extinction.