Table A.1
Data for the calculation of the literature FIP bias.
| Star | Corona | Photosphere | FIP bias | Corona | Solar photosphere | ||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| [C/Fe] | [N/Fe] | [O/Fe] | [Ne/Fe] | [C/Fe] | [N/Fe] | [O/Fe] | [Ne/Fe] | source | source | ||
| AD Leo | 1.45 | 0.96 | 1.64 | 1.18 | 0.93 | 0.33 | 1.19 | 0.80 | 0.49 ± 0.11 | (1) | (30) |
| CN Leo | 1.25 | 0.64 | 1.33 | 0.76 | 0.93 | 0.33 | 1.19 | 0.80 | 0.27 ± 0.17 | (2) Table 2 DEM1 | (24) |
| EQ Peg A | – | 0.80 | 1.68 | 1.17 | – | 0.33 | 1.19 | 0.80 | 0.53 ± 0.07 | (3) Table 7 Q | (25) |
| EQ Peg B | – | 0.82 | 1.61 | 1.13 | – | 0.33 | 1.19 | 0.80 | 0.49 ± 0.08 | (3) Table 7 Q | (25) |
| Prox Cen | – | 1.13 | 1.54 | 1.04 | – | 0.33 | 1.19 | 0.80 | 0.55 ± 0.30 | (3) Table 10 Q | (25) |
| EV Lac | – | 0.93 | 1.69 | 1.10 | – | 0.33 | 1.19 | 0.80 | 0.55 ± 0.15 | (3)Table 10 Q | (25) |
| YY Gem | – | 1.12 | 1.75 | 1.26 | – | 0.33 | 1.19 | 0.80 | 0.69 ± 0.17 | (3) Table 10 Q | (25) |
| AU Mic | 1.63 | 1.19 | 1.77 | 1.39 | 0.93 | 0.33 | 1.19 | 0.80 | 0.68 ± 0.13 | (1) | (30) |
| AT Mic | 1.42 | 0.82 | 1.55 | 1.16 | 0.93 | 0.33 | 1.19 | 0.80 | 0.51 ± 0.07 | (4) Table 4 3T model | (24), O, Fe (26) |
| AB Dor | 1.50 | 1.06 | 1.75 | 1.35 | 0.93 | 0.33 | 1.19 | 0.80 | 0.60 ± 0.09 | (1) | (30) |
| LO Peg | 1.50 | 0.84 | 1.61 | 1.35 | 0.93 | 0.33 | 1.19 | 0.80 | 0.59 ± 0.07 | (5) Table 1 Q | (26) |
| V471 Tau | – | – | 1.57 | 1.04 | – | – | 1.19 | 0.80 | 0.39 ± 0.10 | (6) Table 4 | (26), O (27) |
| 36 Oph A | 0.57 | 0.44 | 1.19 | 0.88 | 0.83 | 0.49 | 1.35 | 0.96 | − 0.14 ± 0.09 | (1) | (30), ph. a. (33) |
| 36 Oph B | 0.44 | 0.33 | 1.10 | 0.67 | 0.83 | 0.49 | 1.35 | 0.96 | − 0.27 ± 0.10 | (1) | (30), ph. a. (33) |
| ξ Boo B | 0.78 | – | 1.19 | 0.97 | 1.09 | – | 1.36 | 0.97 | − 0.16 ± 0.15 | (1) | (30), ph. a. (33) |
| 61 Cyg A | 0.95 | 0.34 | 1.12 | 0.79 | 0.93 | 0.33 | 1.19 | 0.80 | − 0.01 ± 0.04 | (1) | (30), ph. a. (35) |
| 61 Cyg B | 1.26 | – | 1.60 | 1.06 | 0.93 | – | 1.19 | 0.80 | 0.33 ± 0.08 | (1) | (30), ph. a. (35) |
| 70 Oph A | 0.64 | 0.18 | 0.92 | 0.56 | 0.88 | 0.41 | 1.27 | 0.88 | − 0.29 ± 0.06 | (1) | (30), ph. a. (33) |
| 70 Oph B | 0.98 | 0.70 | 1.35 | 1.01 | 0.88 | 0.41 | 1.27 | 0.88 | 0.15 ± 0.10 | (1) | (30), ph. a. (33) |
| ϵ Eri | 0.90 | 0.42 | 1.20 | 0.84 | 0.75 | 0.35 | 1.21 | 0.82 | 0.06 ± 0.07 | (1) | (30), ph. a. (33) |
| α Cen A | 0.72 | 0.06 | 0.35 | 0.41 | 0.99 | 0.46 | 1.32 | 0.93 | − 0.54 ± 0.30 | (1) low activity | (30), ph. a. (33) |
| α Cen B | 0.70 | 0.14 | 0.87 | 0.33 | 0.94 | 0.43 | 1.29 | 0.90 | − 0.38 ± 0.15 | (1) low activity | (30), ph. a. (33) |
| π1 UMa | 0.54 | 0.36 | 0.84 | 0.48 | 1.07 | 0.54 | 1.40 | 1.01 | − 0.45 ± 0.18 | (1) | (30), ph. a. (33) |
| EK Dra | 0.98 | 0.19 | 1.12 | 0.96 | 0.93 | 0.33 | 1.19 | 0.80 | − 0.00 ± 0.13 | (1) | (30) |
| ξ Boo A | 0.75 | 0.20 | 1.11 | 0.69 | 1.09 | 0.50 | 1.36 | 0.97 | − 0.29 ± 0.04 | (1) | (30), ph. a. (33) |
| χ1 Ori | 0.35 | − 0.33 | 0.64 | 0.49 | 0.99 | 0.48 | 1.34 | 0.56 | − 0.47 ± 0.33 | (7) | (24), Fe (28), ph. a. (29) |
| κ Cet | 0.42 | − 0.12 | 0.67 | 0.61 | 1.03 | 0.48 | 1.34 | 0.56 | − 0.38 ± 0.34 | (7) | (24), Fe (28), ph. a. (29) |
| β Com | 0.49 | − 0.53 | 0.59 | 0.07 | 0.96 | 0.46 | 1.32 | 0.54 | − 0.58 ± 0.25 | (7) | (24), Fe (28), ph. a. (29) |
| 47 Cas B | 0.83 | 0.39 | 1.03 | 1.03 | 0.93 | 0.33 | 1.19 | 0.41 | 0.19 ± 0.36 | (7) | (24), Fe (28) |
| ι Hor | 0.75 | 0.43 | 1.31 | 0.79 | 0.95 | 0.30 | 1.16 | 0.38 | 0.21 ± 0.25 | (8) | (30) |
| 11 LMi | 0.97 | 0.11 | 1.09 | 0.33 | 0.93 | 0.33 | 1.19 | 0.80 | − 0.10 ± 0.22 | (9) Table 3 | (30) |
| HR 7291 | – | – | 0.68 | 0.13 | – | – | 1.19 | 0.80 | − 0.51 ± 0.12 | (9) Table 4 | (30) |
| σ2 CrB | – | 0.35 | 1.17 | 0.74 | – | 0.33 | 1.19 | 0.80 | 0.06 ± 0.04 | (10) Table 5 Q | (26) |
| ξ UMa | – | – | 1.42 | 1.11 | – | – | 1.19 | 0.80 | 0.35 ± 0.05 | (11) Table 3 | (26) |
| HR 1099 | 1.50 | 1.16 | 1.87 | 1.41 | 0.93 | 0.33 | 1.19 | 0.80 | 0.76 ± 0.12 | (12) Table 4 APEC | (24), Fe (28) |
| UX Ari | 1.95 | 1.72 | 2.03 | 1.72 | 0.93 | 0.33 | 1.19 | 0.80 | 1.13 ± 0.25 | (12) Table 4 APEC | (24), Fe (28) |
| λ And | 1.28 | 0.74 | 1.67 | 1.31 | 0.93 | 0.33 | 1.19 | 0.80 | 0.52 ± 0.07 | (12) Table 4 APEC | (24), Fe (28) |
| VY Ari | 1.57 | 1.11 | 1.78 | 1.44 | 0.93 | 0.33 | 1.19 | 0.80 | 0.74 ± 0.09 | (12) Table 4 APEC | (24), Fe (28) |
| Capella | 0.66 | 0.40 | 0.93 | 0.40 | 0.93 | 0.33 | 1.19 | 0.80 | − 0.13 ± 0.20 | (12) Table 4 APEC | (24), Fe (28) |
| σ Gem | – | 1.21 | 1.61 | 1.24 | – | 0.33 | 1.19 | 0.80 | 0.66 ± 0.26 | (13) Table 4 | rel. to same solar |
| 31 Com | – | – | 1.31 | 0.66 | – | – | 1.19 | 0.80 | 0.07 ± 0.19 | (14) Table 5 | (25) |
| μ Vel | – | – | 1.06 | 0.44 | – | – | 1.19 | 0.80 | − 0.16 ± 0.16 | (14) Table 5, ObsID 3410 | (25) |
| β Cet | – | – | 1.13 | 0.54 | – | – | 1.19 | 0.80 | − 0.08 ± 0.14 | (14) Table 5 | (25) |
| FK Com | – | – | 1.35 | 1.06 | – | – | 1.19 | 0.80 | 0.29 ± 0.07 | (15) Table 7 | (24) |
| YY Men | 1.14 | 1.19 | 1.41 | 1.13 | 0.93 | 0.33 | 1.19 | 0.80 | 0.49 ± 0.31 | (16) Table 2 XMM Method 1 | (26) |
| EI Eri | 0.10 | 0.25 | 0.15 | 0.08 | 0.00 | 0.00 | 0.00 | 0.00 | 0.23 ± 0.08 | (17) Figure 5 | (30) |
| V851 Cen | 1.19 | 1.05 | 1.84 | 1.50 | 0.93 | 0.33 | 1.19 | 0.80 | 0.67 ± 0.22 | (18) Table 2 | (24) |
| AR Psc | 1.74 | 1.00 | 1.70 | 1.18 | 0.93 | 0.33 | 1.19 | 0.80 | 0.68 ± 0.19 | (19) Table 5 | (25) |
| AY Cet | 1.70 | 1.01 | 1.37 | 0.96 | 0.93 | 0.33 | 1.19 | 0.80 | 0.53 ± 0.32 | (19) Table 5 | (25) |
| II Peg | – | 1.33 | 2.47 | 1.93 | – | 0.33 | 1.19 | 0.80 | 1.22 ± 0.14 | (20) Table 4 Q | (24) |
| AR Lac | – | 0.93 | 1.51 | 1.10 | – | 0.33 | 1.19 | 0.80 | 0.49 ± 0.17 | (21) Table 3 | (24) |
| η Lep | 0.78 | – | 1.09 | 0.55 | 1.03 | – | 1.35 | 0.96 | − 0.31 ± 0.09 | (1) | (30), ph. a. (32) |
| π3 Ori | 0.79 | 0.11 | 0.92 | 0.46 | 1.12 | 0.49 | 1.35 | 0.96 | − 0.41 ± 0.07 | (1) | (30), ph. a. (33) |
| τ Boo A | 0.83 | – | 0.91 | 0.50 | 0.93 | – | 1.16 | 0.77 | − 0.21 ± 0.09 | (1) | (30), ph. a. (34) |
| Procyon | 1.20 | 0.68 | 1.43 | 0.77 | 0.93 | 0.33 | 1.19 | 0.80 | 0.29 ± 0.17 | (22) Table 4 | (24), Fe=7.51 |
| Altair | 0.95 | 0.32 | 0.96 | 0.26 | 1.06 | 0.89 | 1.75 | 1.36 | − 0.56 ± 0.42 | (23) Table 2 MOS/RGS | (26), ph. a. (31) |
Notes. Coronal abundances are taken in quiescent- (Q) or low-activity state, where available. The original assumed solar photospheric values are indicated in the last column, which were all converted to Asplund et al. (2009) and Ne from Drake & Testa (2005). If there were available stellar photospheric abundance (ph. a.) measurements for a star, the source is also given in the last column. The FIP bias and its uncertainty are calculated as the mean and standard deviation of [X/Fe]cor−[X/Fe]phot, where X can be C, N, O, and Ne. The FIP bias column is corrected by +0.084 according to Wood et al. (2018), except for the stars listing (1) as source. As discussed in Sect. 2, GJ 338 AB is omitted.
References. (1) Wood et al. (2018), (2) Fuhrmeister et al. (2007), (3) Liefke et al. (2008), (4) Robrade & Schmitt (2005), (5) Lalitha et al. (2017), (6) García-Alvarez et al. (2005), (7) Telleschi et al. (2005), (8) Sanz-Forcada et al. (2019), (9) Peretz et al. (2015), (10) Osten et al. (2003), (11) Ball et al. (2005), (12) Audard et al. (2003), (13) Huenemoerder et al. (2013), (14) García-Alvarez et al. (2006), (15) Gondoin et al. (2002), (16) Audard et al. (2004), (17) Nordon et al. (2013), (18) Sanz-Forcada et al. (2004), (19) Sanz-Forcada et al. (2009), (20) Huenemoerder et al. (2001), (21) Huenemoerder et al. (2003), (22) Raassen et al. (2002), (23) Robrade & Schmitt (2009), (24) Anders & Grevesse (1989), (25) Asplund et al. (2005), (26) Grevesse & Sauval (1998), (27) Allende Prieto et al. (2001), (28) Grevesse & Sauval (1999), (29) Allende Prieto et al. (2006), (30) Asplund et al. (2009), (31) Erspamer & North (2003), (32) Yüce et al. (2011), (33) Allende Prieto et al. (2004), (34) Gonzalez & Laws (2007), (35) Jofré et al. (2015)
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