1998A&A...332..224H


Query : 1998A&A...332..224H

1998A&A...332..224H - Astronomy and Astrophysics, volume 332, 224-234 (1998/4-1)

Metal abundances of A-type stars in galactic clusters. II. Pleiades, Coma Berenices, Hyades, and Praesepe.

HUI-BON-HOA A. and ALECIAN G.

Abstract (from CDS):

A study of chemical composition for 23 A-type stars in four nearby open clusters (Pleiades, Coma, Hyades and Praesepe) has derived detailed abundances for Mg, Ca, Sc, Cr, Fe, and Ni from high resolution spectroscopy. These results are discussed using the microscopic diffusion model, which yields time-dependent element stratifications as in the case of Am stars. For the Pleiades, the youngest cluster, we find several atypical abundance patterns, which may be transient phases of the Am phenomenon. The members of the older clusters show globally more classical patterns.

Abstract Copyright:

Journal keyword(s): open clusters: individual: Pleiades, Coma Berenices, Hyades, Praesepe - stars: abundances - chemically peculiar

Simbad objects: 27

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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 - 2024
#notes
1 HD 22615 V* 03 39 00.0585760560 +20 54 56.784028824   6.646 6.493     A4III 61 0
2 V* V624 Tau dS* 03 43 43.2412431936 +24 22 28.445642868   8.49 8.22     A7V 125 0
3 V* V1187 Tau dS* 03 44 00.2690335032 +24 33 25.193571588   8.28 8.07     A5V 135 0
4 HD 23325 Pe* 03 45 06.5388153048 +24 15 48.650236236   8.96 8.70   8.16 kA6hA9mF1(IV) 99 0
5 HD 23387 ** 03 45 37.7883282408 +24 20 08.303093844   7.33 7.19   6.96 A1V 123 0
6 Cl Melotte 22 OpC 03 46 24.2 +24 06 50           ~ 3435 0
7 V* V647 Tau dS* 03 47 19.3458598776 +24 08 20.815318464   8.51 8.26   7.97 A7Vs 164 0
8 HD 23610 SB* 03 47 22.8997617600 +22 55 19.586180208   8.41 8.20   7.83 A3/7 65 0
9 HD 23631 SB* 03 47 24.4137493776 +23 54 52.826531688   7.34 7.30   7.11 A0V 121 0
10 HD 23924 * 03 49 40.9233801600 +23 20 29.652869940   8.32 8.13   7.91 A5VkA7mA7 105 0
11 * 63 Tau SB* 04 23 25.0640719200 +16 46 38.150834016   5.957 5.625 7.04 5.33 A1m 290 0
12 * del02 Tau PM* 04 24 05.7614531616 +17 26 38.871301956 5.07 4.95 4.80 4.64 4.57 A2Vs 240 0
13 * del03 Tau a2* 04 25 29.3847186643 +17 55 40.463442784   4.369 4.298 6.18 4.24 A2IV-Vs 407 0
14 Cl Melotte 25 OpC 04 29 47.3 +16 56 53           ~ 3074 0
15 * 81 Tau SB* 04 30 38.8891193184 +15 41 30.760430964   5.739 5.454 6.76   Am 211 0
16 HD 30210 PM* 04 46 01.7404096416 +11 42 20.112329592   5.566 5.346     Am 160 0
17 * h Ori SB* 05 09 19.6432730712 +09 49 46.502673924 5.83 5.67 5.43 5.25 5.13 A2m 251 0
18 HD 72942 SB* 08 36 17.4427895592 +20 20 29.417866260   7.60 7.48     A3V 78 0
19 HD 73174 SB* 08 37 36.9991109064 +19 43 58.510939908   7.95 7.76     Am 90 0
20 NGC 2632 OpC 08 40 13.0 +19 37 16           ~ 1564 0
21 HD 73712 SB* 08 40 20.1451748712 +19 20 56.315955804   7.04 6.78     A9V 101 0
22 HD 73730 V* 08 40 23.4641462184 +19 50 05.895548772   8.20 7.99     F2III 81 0
23 * 8 Com * 12 19 19.1929880208 +23 02 04.821806040   6.416 6.220     A8m 138 0
24 Cl Melotte 111 OpC 12 24 03.4 +25 39 07           ~ 480 0
25 * 13 Com a2* 12 24 18.5489029728 +26 05 54.921403788   5.26 5.18     A3V 143 0
26 HD 108486 EB* 12 27 38.3636590224 +25 54 43.580490048   6.835 6.654     A1IV-VSrSi 127 0
27 * 22 Com * 12 33 34.2193153104 +24 16 58.739975472   6.363 6.243     A4Vm 155 0

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