Table 2.
Catalog of sources with extinction, distance, or object classification results.
| Src | RA | Dec | Literature | K | Matched | Pop. | Cl05 | Rint | AV(d) | rest | Source |
|---|---|---|---|---|---|---|---|---|---|---|---|
| # | (20h) | (+37°) | identifier (a) | (mag) | observ. (b) | reg. (c) | (mag) | (kpc) | classif. (e) | ||
| 1 | 21:15.34 | 24:30.9 | HD 229059 | 4.865 | CGOS | LRP | Out | 0.991 | 5.08 |
 |
B2Iabe |
| 2 | 21:23.80 | 20:01.4 | 6.290 | GOS | LRP | Out | 0.848 |
 |
|||
| 3 | 21:56.20 | 21:28.5 | HD 229105 | 6.886 | GOS | LRP | Out | 0.780 | 0 |
 |
K2II |
| 4 | 22:14.61 | 16:14.7 | 6.940 | GOS | LRP | Out | 0.757 |
 |
|||
| 5 | 21:35.54 | 23:29.6 | BD+36.4031 | 7.107 | GOS | LRP | Out | 0.787 | 0 |
 |
K0III |
| 6 | 21:34.04 | 23:53.1 | 7.264 | GOS | LRP | Out | 0.731 |
 |
|||
| 7 | 21:46.38 | 15:37.0 | 7.334 | GOS | LRP | Out | 1.021 |
 |
|||
| 8 | 21:50.52 | 28:57.0 | 7.411 | GOS | LRP | Out | 0.794 |
 |
|||
| 9 | 21:38.66 | 25:15.0 | BD+36.4032 | 7.455 | CGOS | LRP | In | 1.000 | 4.34 |
 |
O8.5-9III-V |
| 10 | 21:33.56 | 24:51.4 | V439 Cyg | 7.629 | GOS | LRP | Out | 1.489 | 4.28 |
 |
B1.5Ve |
| 11 | 21:37.02 | 24:17.1 | 7.811 | OS | HRP | Out | 0.735 | 19.45 | |||
| 12 | 22:07.64 | 28:12.3 | 7.845 | GOS | HRP | Out | 0.717 | 7.12 | |||
| … | … | … | … | … | … | … | … | … | … | … | … |
Notes. The full version of this table is available at the CDS. Objects are sorted by K-band magnitude or by RA when K is lacking.
This identifier can be either a SIMBAD ID or “Cygnus 2N” and “Cygnus 2N EAST” for the so-called components as described in Sect. 2.6 or “Sk19 Ta-bb”, standing for (Skinner et al. 2019, Table a, line bb).
List of observations where a counterpart has been found, coded as C = Chandra, likely counterpart; c = Chandra, doubtful counterpart; G = Gaia; O = OMEGA2000 (even when 2MASS is used for photometry instead); S = Spitzer; H = Herschel.
Source inside or outside the Cl05 region (as defined in Sect. 3.1).
This column either shows the known spectral type or our classification as YSO candidate according to the following abbreviations: cI, class I; cII, class II; cIII, class III; c.protost., candidate protostar; c.starless, candidate starless core; massiveSF, massive star-forming region; othX, other X-ray-detected candidate; Rint: identified through the Rint method; YSOc, YSO candidate.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.