1999PASP..111..335W

Query : 1999PASP..111..335W

1999PASP..111..335W - Publ. Astron. Soc. Pac., 111, 335-341 (1999/March-0)

The CaII-Mv correlation (Wilson-Bappu effect) calibrated by Hipparcos parallaxes.

WALLERSTEIN G., MACHADO-PELAEZ L. and GONZALEZ G.

Abstract (from CDS):

We have used Hipparcos parallaxes to derive absolute visual magnitudes of G, K, and M stars with Ca II emission line widths previously measured by O. C. Wilson. A linear relationship similar to the one derived originally by Wilson & Bappu and improved by Lutz & Kelker was found from Mv=+7 to -2. For stars brighter than Mv=-2 a substantial number of stars show Ca II emission lines that are broader than expected from the linear fit. Most of those stars are bright giants and supergiants of type G. In appendices we show some sample Ca II profiles and identify emission lines of Fe II as well as the Hε line in some stars.

Abstract Copyright: ∼

Journal keyword(s): Stars: Chromospheres - Stars: Distances - Stars: Fundamental Parameters

VizieR on-line data: <Available at CDS (J/PASP/111/335): table1a.dat table1b.dat table1c.dat + figures>

Simbad objects: 43

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Number of rows : 43
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 * 33 Psc RS* 00 05 20.1411719640 -05 42 27.431698821 6.52 5.65 4.61 3.83 3.29 K0III-IV 208 0
2 V* AD Cet LP? 00 14 27.6308065618 -07 46 49.903268768 8.55 6.74 5.12     M3+III 79 0
3 * chi Peg PM* 00 14 36.1642825005 +20 12 24.130377664 8.280 6.380 4.800 3.45 2.32 M2+III 191 0
4 * 7 Cet LP? 00 14 38.4169134264 -18 55 58.308074157 8.07 6.12 4.46 3.06 1.92 M1III 95 0
5 * iot Cet * 00 19 25.6743948847 -08 49 26.108975369 5.94 4.77 3.55 2.70 2.11 K1+IIICN0.5 180 0
6 HD 1632 * 00 20 45.5169107040 +32 54 40.272404904   7.381 5.794     K5III 39 0
7 * del And SB* 00 39 19.6031132231 +30 51 39.540873571 6.04 4.56 3.28 2.36 1.70 K3III-IIIbCN0.5 328 0
8 * alf Cas PM* 00 40 30.4430418459 +56 32 14.385181354 4.52 3.40 2.23 1.45 0.85 K0-IIIa 339 0
9 * bet Cet PM* 00 43 35.37090 -17 59 11.7827 3.90 3.02 2.01 1.29 0.78 G9.5IIICH-1 525 1
10 * phi01 Cet PM* 00 44 11.4000904231 -10 36 34.382643011   5.773 4.767     K0III 112 0
11 * del Psc PM* 00 48 40.9443145328 +07 35 06.294902124 7.83 5.95 4.44 3.27 2.40 K5-III 187 0
12 * 20 Cet * 00 53 00.4942192605 -01 08 39.335217612 8.24 6.34 4.76 3.55 2.64 K5III 95 0
13 * ups01 Cas PM* 00 55 00.1557027792 +58 58 21.717145956   6.042 4.820     G8III 103 0
14 * eta And SB* 00 57 12.4002792266 +23 25 03.540083245 6.05 5.36 4.42 3.69 3.21 G8-III 189 0
15 HD 6497 PM* 01 07 00.1745063280 +56 56 05.898658776   7.605 6.401     K2III-IV 111 0
16 * 2 UMi PM* 01 08 44.8786355178 +86 15 25.526405536   5.459 4.225     K2III 89 0
17 * bet And PM* 01 09 43.92388 +35 37 14.0075 5.58 3.62 2.05 0.81 -0.19 M0+IIIa 555 1
18 HD 6833 * 01 09 52.2648344184 +54 44 20.278107384 8.81 7.91 6.74     K0IIIbFe-2 195 0
19 * ksi And * 01 22 20.4200755704 +45 31 43.596248844   5.951 4.868     K0-IIIb 132 0
20 * 46 Cet * 01 25 37.2394436400 -14 35 55.626569448   6.138 4.907     K2+III-IIIbCN0.5 72 0
21 * mu. Psc PM* 01 30 11.1150260499 +06 08 37.758162354 7.75 6.22 4.84 3.78 3.04 K3III 179 0
22 HD 9166 PM* 01 32 24.4429815360 +68 24 32.107978116   8.056 6.803     K3III 44 0
23 * 14 Per * 02 44 05.1600277584 +44 17 49.341411348   6.320 5.435     G0Ib-IIaCa1 132 0
24 HD 20123 * 03 16 12.2028107016 +50 56 15.605186388 7.01 6.18 5.03     G5Ib-IIa 95 0
25 * mu. Per SB* 04 14 53.8635146524 +48 24 33.590334394 5.75 5.12 4.16 3.38 2.83 G0Ib 242 0
26 * F Hya * 08 43 40.3744846779 -07 14 01.422508229   5.441 4.625     G1Ib 165 0
27 * gam01 Leo PM* 10 19 58.354462 +19 50 29.35920 4.13 3.13 1.98 1.13 0.51 K1-IIIFe-1 281 1
28 * 37 LMi * 10 38 43.2128104658 +31 58 34.463378806   5.494 4.677     G2.5IIIa 156 0
29 * 56 Leo LP? 10 56 01.4682688998 +06 11 07.341317877 8.45 7.24 5.78 3.53 1.44 M5.5III: 172 0
30 * alf UMa SB* 11 03 43.67152 +61 45 03.7249 3.78 2.86 1.79 0.98 0.40 G9III+A7.5 439 0
31 * nu. Vir LP* 11 45 51.5595979999 +06 31 45.748996439 7.32 5.54 4.04 2.79 1.78 M1III 259 0
32 * p Vir PM* 13 54 42.1451337000 -01 30 11.241795960   6.258 5.159     K1/2II/III 79 0
33 * alf Boo RG* 14 15 39.67207 +19 10 56.6730 2.46 1.18 -0.05 -1.03 -1.68 K1.5IIIFe-0.5 2318 1
34 * 110 Vir PM* 15 02 54.0375635908 +02 05 28.695699730 6.31 5.44 4.40 3.59 3.05 K0+IIIbFe-0.5 126 0
35 * iot Dra V* 15 24 55.7738042889 +58 57 57.837111857 5.68 4.45 3.29 2.51 1.91 K2III 409 1
36 * bet Dra * 17 30 25.9616959 +52 18 04.999351 4.43 3.79 2.81 2.12 1.64 G2Ib-IIa 415 0
37 * bet Sct SB* 18 47 10.4742156840 -04 44 52.342960488 6.15 5.31 4.22 3.43 2.86 G4IIa 187 0
38 * ksi Cyg SB* 21 04 55.8599363125 +43 55 40.272058234 7.17 5.39 3.73 2.55 1.63 K4.5Ib-II 311 0
39 * zet Cap SB* 21 26 40.0306553034 -22 24 40.753242596 5.35 4.75 3.74 3.09 2.65 G4Ib:Ba2 280 1
40 * bet Aqr * 21 31 33.5320760349 -05 34 16.229381029 4.27 3.71 2.89 2.29 1.84 G0Ib 447 0
41 * alf Aqr * 22 05 47.0355458275 -00 19 11.463439527 4.65 3.90 2.94 2.27 1.76 G2Ib 437 0
42 * zet Cep s*r 22 10 51.2777055617 +58 12 04.542602641 6.62 4.90 3.35 2.27 1.49 K1.5Ib 278 0
43 * 104 Aqr * 23 41 45.8063762520 -17 48 59.515007076 6.14 5.65 4.83 4.22 3.80 G2Ib/II 105 0

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