Table 1.
Information on giant members of NGC 6866.
| KIC ID | KIC 8461659 | KIC 8329894 | KIC 8395903 | KIC 8264549 | KIC 7991875 | KIC 8264592 |
|---|---|---|---|---|---|---|
| Symbol in plots | Cross | Square | Circle | Triangle | Star | Diamond |
| Gaia DR3 ID | 208189159- | 207606690- | 208207250- | 207587768- | 207586586- | 207587709- |
| 4650263424 | 1752525440 | 2978527488 | 2673012480 | 2922829056 | 8557450112 | |
| 2MASS ID | 20043730 | 20032282 | 20034631 | 20035516 | 20030966 | 20035769 |
| +4425100 | +4415502 | +4422526 | +4408242 | +4346055 | +4406276 | |
| RA (deg) | 301.155417 | 300.845116 | 300.942946 | 300.979852 | 300.790240 | 300.990398 |
| Dec (deg) | 44.419404 | 44.263915 | 44.381256 | 44.140023 | 43.768202 | 44.107644 |
| KS (mag) | 8.760(16) | 9.14(16) | 9.166(14) | 9.235(18) | 8.931(16) | 9.351(16) |
| G (mag) | 11.287534 | 11.302372 | 11.438034 | 11.360455 | 11.102879 | 11.447467 |
| G − KS (mag) | 2.53 | 2.157 | 2.272 | 2.125 | 2.172 | 2.096 |
| GBP − GRP DR3 | 1.4409981 | 1.2247219 | 1.2931328 | 1.1832037 | 1.2294884 | 1.1834383 |
| RV (km s−1) | 12.3 | 12.2 | 12.6 | 14.2 | 12.7 | 13.5 |
| pmra (mas yr−1) | –1.348(12) | –1.163(14) | –1.335(13) | –1.227(33) | –1.316(17) | –1.177(13) |
| pmdec (mas yr−1) | –5.848(12) | –5.728(13) | –5.905(13) | –5.742(32) | –5.855(16) | –6.141(13) |
| Gaia DR3 parallax (mas) | 0.682(11) | 0.652(12) | 0.700(11) | 0.677(29) | 0.659(13) | 0.661(11) |
| ν_eff | 1.4282342 | – | 1.4545882 | 1.4765111 | 1.4668154 | 1.476384 |
| pseudocolour | – | 1.4647219 | – | – | – | – |
| npar | 5 | 6 | 5 | 5 | 5 | 5 |
| ecl_lat (deg) | 62.285942 | 62.244026 | 62.318716 | 62.090355 | 61.814700 | 62.057926 |
| RUWE | 0.8569876 | 0.99588126 | 0.85863876 | 2.0729961 | 0.90071553 | 0.842494 |
| Parallax corr. (mas) | –0.02964 | –0.03021 | –0.03256 | –0.03461 | –0.03004 | –0.03490 |
| Distance (pc) | 1405 | 1466 | 1365 | 1405 | 1451 | 1437 |
| (m − M)0 (mag) | 10.74 | 10.83 | 10.68 | 10.74 | 10.81 | 10.79 |
| P_mem (a) | 0.4 | 0.9 | 0.7 | 0.6 | – | 0.3 |
| Teff (K) (b) | 5044 | 5114 | 5104 | 5201 | – | – |
| Teff (K) (c) | 5045 | – | – | – | – | - |
| Teff (K) (d) | 5032 | 5069 | – | – | – | – |
| Teff (K) (e) | 4983 | – | 5052 | – | 4969 | – |
| Teff (K) (f) | 4998 | 5052 | 5052 | 5052 | – | 5037 |
| Teff (K) (g) | – | 5092 | 5106 | 5126 | – | – |
| Teff from DR3 GBP − GRP (K) (h) | 4864 | 5091 | 5037 | 5106 | 5078 | 4975 |
| Teff from G − KS (K) (i) | 4978 | 5157 | 5120 | 5112 | 5137 | 5037 |
| Teff (K) (j) | 5044 | 5096 | 5101 | 5117 | – | 5105 |
| [M/H] (j) | +0.021 | +0.027 | −0.011 | +0.021 | – | +0.021 |
| [C/N] (j) | −0.636 | −0.522 | −0.535 | −0.608 | – | −0.561 |
| E(B − V) calculated (k) | 0.294 | 0.139 | 0.193 | 0.132 | 0.127 | 0.114 |
| E(B − V) Green (l) |
 |
 |
 |
 |
 |
 |
| E(B − V) from NaD-lines (m) | – | 0.12(2) | 0.24(3) | – | – | 0.12(1) |
| E(B − V) Lallement (n) | 0.173(35) | 0.166(36) | 0.161(34) | 0.156(34) | 0.160(34) | 0.160(33) |
| BCG (mag) | –0.020 | 0.012 | 0.007 | 0.012 | 0.006 | –0.004 |
| BCKS (mag) | 1.933 | 1.841 | 1.857 | 1.841 | 1.861 | 1.891 |
| L(L⊙) from KS | 94.4(3.5) | 70.4(2.9) | 61.1(2.2) | 60.1(5.1) | 81.3(3.5) | 55.7(2.1) |
| R(R⊙) SB | 12.72(56) | 10.76(47) | 10.01(43) | 9.86(57) | 11.81(53) | 9.55(41) |
Notes.
LAMOST DR5, Zhong et al. (2020).
APOKASC, Pinsonneault et al. (2018).
LAMOST, Frasca et al. (2016).
Adopting E(B − V) and requiring bolometric corrections from Casagrande & VandenBerg (2018) to reproduce observed colour. [Fe/H] = +0.0 and log g = 2.7 was assumed. A change of ±0.1 dex in [Fe/H] corresponds to ±17 K, a change of ±0.1 in log g yields ±3 K, and ±0.03 in E(B − V) gives about ±80 K.
As (h), but also using Casagrande & VandenBerg (2014).
APOGEE DR17. Taken from https://skyserver.sdss.org/dr18/SearchTools/IRQS.
Calculated by assuming APOGEE Teffs from (j) and requiring bolometric corrections from Casagrande & VandenBerg (2018, 2014) to yield the observed G − KS.
From Bayestar2019 E(g − r), assuming a mean of the two conversion factors 0.884 and 0.996 given in Green et al. (2019). AG = 2.74 × E(B − V) Casagrande & VandenBerg (2018). AKS = 0.366 × E(B − V) Casagrande & VandenBerg (2014).
Using Munari & Zwitter (1997) and spectra from FIES at the Nordic Optical Telescope.
Using Lallement et al. (2018).
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.