2021A&A...650A.156D


Query : 2021A&A...650A.156D

2021A&A...650A.156D - Astronomy and Astrophysics, volume 650A156-156 (2021/6-1)

Clustered star formation toward Berkeley 87/ON2. I. Multiwavelength census and the population overlap problem.

DE LA FUENTE D., ROMAN-ZUNIGA C.G., JIMENEZ-BAILON E., ALVES J., GARCIA M. and VENUS S.

Abstract (from CDS):


Context. Disentangling line-of-sight alignments of young stellar populations is crucial for observational studies of star-forming complexes. This task is particularly problematic in a Cygnus-X subregion where several components, located at different distances, overlap: the Berkeley 87 young massive cluster, the poorly known [DB2001] Cl05 embedded cluster, and the ON2 star-forming complex, which in turn is composed of several HII regions.
Aims. We provide a methodology for building an exhaustive census of young objects that can consistently treat large differences in extinction and distance.
Methods. OMEGA2000 near-infrared observations of the Berkeley 87/ON2 field were merged with archival data from Gaia, Chandra, Spitzer, and Herschel and with cross-identifications from the literature. To address the incompleteness effects and selection biases that arise from the line-of-sight overlap, we adapted existing methods for extinction estimation and young object classification. We also defined the intrinsic reddening index, Rint, a new tool for separating intrinsically red sources from those whose infrared color excess is caused by extinction. Finally, we introduce a new method for finding young stellar objects based on Rint.
Results. We find 571 objects whose classification is related to recent or ongoing star formation. Together with other point sources with individual estimates of distance or extinction, we compile a catalog of 3005 objects to be used for further membership work. A new distance for Berkeley 87, (1673±17)pc, is estimated as a median of 13 spectroscopic members with accurate Gaia EDR3 parallaxes.
Conclusions. The flexibility of our approach, especially regarding the Rint definition, allows overcoming photometric biases caused by large variations in extinction and distance in order to obtain homogeneous catalogs of young sources. The multiwavelength census that results from applying our methods to the Berkeley 87/ON2 field will serve as a basis for disentangling the overlapped populations.

Abstract Copyright: © ESO 2021

Journal keyword(s): methods: observational - techniques: photometric - catalogs - open clusters and associations: individual: Berkeley 87 - ISM: individual objects: ON2 - stars: formation

VizieR on-line data: <Available at CDS (J/A+A/650/A156): table2.dat tablec1.dat>

Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 27

goto Full paper

goto View the references in ADS

Number of rows : 27
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME NOAO Deep Wide Field reg 14 32 05.75 +34 16 47.5           ~ 430 0
2 HD 229059 s*b 20 21 15.3643937664 +37 24 31.106402136 10.66 10.23 8.70     B2Iabe 102 0
3 LS II +37 73 * 20 21 19.2550073064 +37 23 24.728636868 12.4 12.18 10.92     B0.2III 26 0
4 EM* VES 203 Be* 20 21 24.8520232104 +37 22 48.209423376 13.76 13.42 12.141     B0.5V 27 1
5 Cl Berkeley 87 11 * 20 21 27.8236868544 +37 24 31.241922300   11.51 10.97     F8V 5 0
6 EM* AS 407 Be* 20 21 28.3634733024 +37 26 19.987314072   16.05 14.228 13.79   B2e 17 0
7 Cl Berkeley 87 13 * 20 21 31.5600459840 +37 20 41.414090928 12.53 12.41 11.32     B0.5III: 15 0
8 Cl Berkeley 87 16 * 20 21 33.4756361352 +37 24 19.439590176 15.27 14.72 13.39     B2V 11 0
9 EM* MWC 1015 Be* 20 21 33.5822468448 +37 24 51.700205016 13.75 13.28 11.84     B1.5Ve 61 1
10 Cl Berkeley 87 OpC 20 21 35.0 +37 25 14           ~ 141 0
11 Cl Berkeley 87 18 * 20 21 35.2621023936 +37 29 12.121441368 15.13 14.47 12.84     B1V 10 0
12 BD+36 4031 * 20 21 35.5763189472 +37 23 29.834614824   10.73 9.61     K0III 6 0
13 Hen 3-1885 Em* 20 21 35.8910855616 +37 21 39.606386472   11.26 11.13     A0V 8 0
14 Cl Berkeley 87 24 LP? 20 21 38.0978213760 +37 25 17.211356832 13.19 12.82 11.48     B1Ib 11 0
15 BD+36 4032 Em* 20 21 38.6831894784 +37 25 15.208439844 11.94 11.64 10.30 10.09   O8.5III 29 0
16 Cl Berkeley 87 26 * 20 21 39.6899416032 +37 25 05.582975052 13.63 13.25 11.83     B0.5I 14 0
17 Onsala 2S HII 20 21 41.4 +37 25 44           ~ 41 0
18 [DB2001] Cl 5 Cl* 20 21 41.8 +37 25 50           ~ 2 0
19 OH 075.8+00.3 HII 20 21 43.8 +37 26 39           ~ 95 2
20 GAL 075.78+00.34 cor 20 21 44.00 +37 26 38.0           ~ 131 1
21 WR 142 WR* 20 21 44.3438785440 +37 22 30.544989960   14.39 12.99 12.73 11.04 WO2 134 0
22 Cl Berkeley 87 31 * 20 21 45.8805792072 +37 22 25.660336296 14.1 13.72 12.32     B1V 13 0
23 Cl Berkeley 87 32 * 20 21 47.3420980392 +37 26 31.999589664 13.22 12.91 11.57     B0.5III 14 0
24 [DMA88] HII S HII 20 21.8 +37 26           ~ 8 0
25 HD 229105 V* 20 21 56.2039207464 +37 21 28.627442532   11.19 9.955     K2II 9 0
26 EM* VES 204 Be* 20 21 59.95 +37 26 23.5 14.54 14.02 12.44     B1Ve 19 0
27 NAME Cyg X Cld 20 30 04.7973633 +40 51 36.002197           ~ 962 1

To bookmark this query, right click on this link: simbad:objects in 2021A&A...650A.156D and select 'bookmark this link' or equivalent in the popup menu