2004MNRAS.354..727S


Query : 2004MNRAS.354..727S

2004MNRAS.354..727S - Mon. Not. R. Astron. Soc., 354, 727-736 (2004/November-1)

A population model of the solar neighbourhood thin disc white dwarfs.

SCHROEDER K.-P., PAULI E.-M. and NAPIWOTZKI R.

Abstract (from CDS):

We present a model of the solar neighbourhood (d < 100pc) white dwarf (WD) population and show the resulting effective temperature and mass distribution. Our model parameters, in particular the WD cooling time-scale, are constrained by the models of Chabrier et al. The local initial mass function and star formation rate (SFR, per unit volume in the Galactic plane) of Schröder & Pagel are used for the creation of the synthetic stars from which the WDs originate, as well as the above authors' grid of evolutionary tracks. Furthermore, we consider in detail the significant depletion of the older (and cooler) WDs by dilution into the column, as caused by the dynamics of the `thin disc'.

To verify our synthetic sample, especially the WD cooling time-scale, we study the temperature distribution of a small but nearly complete, volume-limited sample of observed WDs, which we characterize by a single and simple indicator R6300: the number ratio of WDs with Teff< 6300K over those with Teff> 6300K. After determination of the bias owing to a residual incompleteness with cool WDs, we find a corrected value of R6300 of 0.68 (±0.24). This is in good agreement with our WD population model: its temperature distribution yields R6300= 0.77.

For a spherical volume around the Sun, with d < 100pc, our population model suggests a total of about 13700 WDs (omiting part of the WDs with a binary system origin, an estimated 7±2 per cent of the total count). A subsample, limited to magnitude 19.0 (as expected for the European Space Agency mission Gaia), would contain about 7750 WDs of this population model. With a less deep magnitude limit of B= 16.0, more typical of current observed WD samples (SN Ia Progenitor surveY; SPY), the number of objects is reduced to only ~1350. We use this specific synthetic subsample to test the completeness of the prospective SPY WD sample, which (with over 50 per cent of the candidates now observed) is already the largest sample of WDs with high-resolution spectra. We find that within d < 100pc and for B < 16.0 SPY will deliver a fairly complete (almost 80 per cent) sample.


Abstract Copyright: 2004 RAS

Journal keyword(s): stars: evolution - white dwarfs - Galaxy: disc - Galaxy: kinematics and dynamics

CDS comments: In Table 3 : WD 2336+079 is a misprint fo WD 2336-079.

Simbad objects: 109

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Number of rows : 109
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 LAWD 96 WD* 00 02 10.7241976499 -43 09 55.390578662   13.12 13.05     DAP5.8 134 0
2 LAWD 1 WD* 00 02 40.0947866937 -34 13 39.592411637   15.36 14.94     DC 75 0
3 EGGR 381 WD* 00 12 14.7449947981 +50 25 20.736275736   14.6   14.2   DA7.6 106 0
4 G 158-45 WD* 00 14 12.7919361867 -13 11 01.087005764   16.48 15.88     DC8H 65 0
5 EGGR 246 WD* 00 41 26.0270023159 -22 21 02.292155084   15.25 14.60 14.088 13.671 DQ9 120 0
6 Wolf 28 WD* 00 49 09.8983373329 +05 23 18.993828947 12.984 12.92 12.374 12.106 11.854 DZ7.5 266 0
7 Wolf 1516 WD* 01 18 00.0751414753 +16 10 20.561712526   13.96   13.9   DC6 101 0
8 LAWD 10 WD* 01 37 59.3936818351 -04 59 44.668541360   13.20 12.83 12.8   DA+D1 191 0
9 L 88-59 WD* 01 43 00.9833777734 -67 18 30.353062494   14.33 13.90 13.52 13.23 DA8.1 76 0
10 EGGR 268 WD* 01 51 51.1387595810 +64 25 52.547329311   13.6   12.8   DA5.6 58 0
11 GD 279 WD* 01 52 02.9620032216 +47 00 06.651152568 11.906 12.519 12.463 12.519 12.586 DA3.6 109 0
12 EGGR 168 WD* 02 11 20.8420869594 +39 55 21.516404474   14.80 14.50 14.4   DAZ6.9 121 0
13 EGGR 16 WD* 02 16 58.0227724350 +42 58 05.242149904   16.96 16.23 16.3   DA9.5 66 0
14 EGGR 471 WD* 02 32 37.9054932741 -14 11 51.767255899   16.51 15.76     DC9 55 0
15 PG 0235+064 WD* 02 38 30.9280475928 +06 37 59.842540308   15.53 15.09     DA3.5 44 0
16 EGGR 473 WD* 02 48 36.4291217434 +54 23 22.464606271   16.25   15.1   DAZ9 73 0
17 CPD-69 177 WD* 03 10 31.0195960176 -68 36 03.380768388 10.757 11.413 11.394 11.47 11.558 DA3.0 299 0
18 L 227-140 PM* 03 12 46.6789814640 -54 06 29.764759608   15.27 14.73 14.81   F5V 16 1
19 EGGR 566 WD* 03 25 11.0474878302 -01 49 15.047041848   16.8 16.22     DZA9 89 0
20 LAWD 14 WD* 03 28 48.7986016948 -27 19 00.096684530   14.0 13.56     DA5.4 81 1
21 Wolf 219 WD* 03 44 34.8473315202 +18 26 09.820674151   15.50   14.8   DQ8 90 0
22 G 7-16 WD* 04 00 26.6831052624 +08 14 06.930002800   16.62   15.4   DC9 54 0
23 * omi02 Eri B WD* 04 15 21.7957181469 -07 39 29.203986789 9.147 9.83 9.53     DA2.9 357 0
24 V* RR Cae WD* 04 21 05.5631820426 -48 39 07.061113433 14.50 14.92 14.40     DA7.8 168 1
25 EGGR 169 WD* 04 25 53.7276237576 +12 11 48.337246428   15.96 15.44 15.54 14.77 DA8 60 0
26 EGGR 180 WD* 04 31 12.5714396826 +58 58 41.292707803 12.29 12.77   12.8   DC5 140 0
27 HD 283750B WD* 04 36 44.8959324504 +27 09 51.523283628   16.46   15.4   DC8 101 0
28 EGGR 41 WD* 04 37 47.4072688697 -08 49 10.619853645   14.24 14.10     DQ8 96 0
29 KUV 05097+1649 V* 05 12 33.5382461760 +16 52 09.225535152   14.94 14.40 14.32   F2V 18 1
30 GD 69 WD* 05 36 20.2147083168 +41 29 55.622008464   15.07 14.75     DA6.5 58 0
31 EGGR 248 WD* 05 51 19.4818569216 -00 10 21.107152956   15.06 14.60     DQ8P 165 0
32 M 37 OpC 05 52 18.6 +32 32 36           ~ 436 0
33 EGGR 45 WD* 05 55 09.5304871511 -04 10 07.065341021   15.49 14.45 13.994 13.538 DZ11 125 0
34 EGGR 290 WD* 05 56 25.4599888487 +05 21 48.443176471   14.77 14.13 14.00   DA8P 163 0
35 G 106-51B WD* 06 30 38.5997399928 -02 05 50.485413624     15.32 15.43   DA7.3 40 0
36 * alf CMa B WD* 06 45 09.3041925037 -16 43 00.724740067   8.41 8.44     DA1.9 563 1
37 EGGR 484 WD* 06 47 22.1508576098 +02 31 08.914947169   16.00   15.7   DA7.0 60 0
38 LAWD 23 WD* 06 47 37.9897150309 +37 30 57.066665144   11.97 12.07 12.26   DA2.3 182 0
39 EGGR 485 WD* 07 00 51.6637780968 +31 57 43.832015694   17.53   15.7   DC10 53 0
40 L 886-6 WD* 07 01 54.8387102144 -06 27 46.230821653   16.2 15.42     DA7.6 50 0
41 G 107-70 ** 07 30 47.30952 +48 10 26.6124 16.01 15.61   14.4   DA+DA 98 0
42 EGGR 321 WD* 07 33 30.8802796728 +64 09 27.434704716   16.4   15.6   DA11P 57 0
43 * alf CMi B WD* 07 39 17.8800 +05 13 26.800   10.7 10.92     DQZ 174 0
44 LAWD 25 WD* 07 40 20.7886676070 -17 24 49.156867583   13.36 13.061 12.886 12.70 DZQA6 218 0
45 VB 3 WD* 07 45 38.4274938131 -33 55 51.341406846   17.40 16.70 16.21 15.23 DC10 51 0
46 EGGR 426 WD* 07 50 14.5843350628 +07 11 48.917000372   17.9   16.2   DC9 74 0
47 EGGR 427 WD* 07 50 15.3418409575 +07 11 37.097929321   17.6   16.1   DC9 72 0
48 LAWD 26 WD* 07 53 08.1439021017 -67 47 31.382011435   14.75 14.09     DA9.0 118 0
49 NGC 2632 OpC 08 39 58.4 +19 36 33           ~ 1733 0
50 CD-32 5613 WD* 08 41 32.4290850497 -32 56 32.915823461   12.07 11.85 12.3   DA5.5 325 0
51 EGGR 250 WD* 09 15 56.0774298887 +53 25 23.857612513   14.09   14.1   DCP7 157 0
52 EGGR 431 Em* 09 41 59.3216028696 +06 57 17.181979848   15.21 14.90     dF 27 1
53 L 190-21 PM* 10 14 58.4198667696 -56 11 11.389286364   15.74 15.03 14.90   F3V 19 0
54 EGGR 350 WD* 10 23 09.0629848950 +63 27 41.489054140   15.09   14.6   DA7.3 70 0
55 LP 37-186 WD* 10 37 02.4755594097 +71 10 58.705020158   17.3   16.1   DC9 44 0
56 EGGR 535 WD* 10 38 55.5700182462 -20 40 56.834110426   15.9 16.28 15.54 15.34 DQ10P 98 0
57 BD-18 3019B WD* 10 45 39.0428670370 -19 06 45.026254097     15.5 15.75   DQ 61 0
58 LAWD 34 WD* 10 57 35.1341950895 -07 31 23.176779615 14.078 14.626 14.338 14.132 13.921 DC 91 0
59 Ross 627 WD* 11 24 12.9710801226 +21 21 35.569805995       14.28   DA6.8 124 0
60 * 20 Crt B WD* 11 34 30.4777605856 -32 50 02.404764059   17 15     DC 53 0
61 GD 140 WD* 11 37 05.1041466528 +29 47 58.288741080 11.47 12.42 12.45 12.73 12.714 DA2.2 257 0
62 LAWD 37 WD* 11 45 42.9169346379 -64 50 29.461957832 11.08 11.725 11.513 11.34 11.163 DQ 287 0
63 WG 21 WD* 12 26 42.0226230528 -66 12 18.467291952   14.37 13.97     DA6.6 51 0
64 WG 22 WD* 12 38 49.7811220835 -49 48 00.219515411   14.14 13.96     DA4.2 245 0
65 Wolf 457 WD* 13 00 09.0631835435 +03 28 41.063241871 16.356 16.452 15.808 15.429 15.044 DAQZ8 108 0
66 EGGR 436 WD* 13 08 41.1944602216 +85 02 28.161666517   16.76   15.9   DA9P 61 0
67 NAME ER 8 WD* 13 12 56.4722073575 -47 28 07.912819252   18.45 17.11 16.32 15.72 DC 46 0
68 BD-07 3632 WD* 13 30 13.6370112733 -08 34 29.468140653 11.803 12.398 12.340 12.39 12.436 DA3.5 203 0
69 Wolf 489 WD* 13 36 31.8521839520 +03 40 45.942173346   15.66   14.48   DC9 128 0
70 EGGR 360 WD* 13 47 24.3696354602 +10 21 38.013189353   15.49   14.8   DA7.1 104 0
71 EGGR 438 WD* 13 48 03.0103253113 +23 34 46.443561286   16.72   15.2   DC9 82 0
72 LP 801-9 WD* 14 47 25.3408507940 -17 42 15.755350506   17.42 16.46     DC10 48 0
73 HD 140901B WD* 15 47 30.0209908033 -37 55 08.460010675   13.10 12.80 13.53 12.34 DA4.8 108 0
74 EGGR 117 WD* 16 11 25.6063713071 +13 22 17.937724651   15.33   15.2   DA5.4 85 0
75 CD-38 10980 WD* 16 23 33.8380498896 -39 13 46.161043572 9.916 10.885 11.029 10.936 10.841 DA2 526 0
76 Ross 640 WD* 16 28 25.0030896166 +36 46 15.846877416   14.01   13.9   DZ6 220 0
77 EGGR 258 WD* 16 34 21.5518633862 +57 10 08.868180953       14.770   DQ8 132 0
78 PG 1633+434 WD* 16 35 01.4291783063 +43 17 36.347179696   15.26   14.5   DAZ7.6 85 0
79 V* DN Dra WD* 16 48 25.6318375106 +59 03 22.658985521   12.34 12.17 12.44   DA4.0 228 0
80 EGGR 494 WD* 17 08 07.9651989788 +02 57 37.081283576   15.65   14.5   DZ7 72 0
81 [RWW88] SC 171751.1-343026 WD* 17 21 10.3222534608 -34 33 28.666355652   17.29 16.38     DA2.0 14 0
82 EGGR 372 WD* 17 48 07.9928195849 +70 52 35.922050086       13.5   DQ9P 153 0
83 EGGR 199 WD* 17 49 50.1474575152 +82 46 26.061955719   14.92   14.5   DA6.8 94 0
84 G 227-28 WD* 18 21 19.8310303352 +61 01 07.383349520   16.62   15.0   DA10 61 0
85 EGGR 374 WD* 18 30 20.2711538874 +54 47 27.207896312   15.99   14.9   DQ7P 101 0
86 LAWD 73 WD* 19 00 10.2533239461 +70 39 51.416733790   13.24   13.5   DAP4.5 264 0
87 EGGR 375 WD* 19 18 58.6307251776 +38 43 21.479206332   15.02   14.1   DC7 83 1
88 LAWD 74 WD* 19 20 34.9229289504 -07 40 00.065957592 11.553 12.345 12.290 12.229 12.164 DBQA5 250 0
89 GD 219 WD* 19 21 40.4179321464 +14 40 41.404467612   13.07 13.01 13.3   DA3.3 92 0
90 V* PY Vul WD* 19 37 13.7502269447 +27 43 18.733503670   13.14   12.7   DA4.0 138 0
91 LAWD 79 WD* 19 56 29.2263375910 -01 02 32.671070269   13.89 13.56 13.73   DA6.4 158 0
92 EGGR 498 WD* 20 05 34.8732768746 -10 56 54.432926709   17.91 16.89 16.4   DA10 59 0
93 LAWD 80 WD* 20 10 17.5214260072 -21 46 45.798289597   14.60 14.58 14.5   DA5.0 59 0
94 CD-30 17706 WD* 20 10 56.8486912016 -30 13 06.627142663 11.654 12.286 12.242 12.311 12.381 DA3.1 267 0
95 HD 340611 WD* 20 34 21.8847019255 +25 03 49.750446346 10.687 11.471 11.546 11.648 11.728 DA2.4 329 0
96 EGGR 261 WD* 20 49 06.6996392736 +37 28 14.050387020   13.40   13.2   DA3.4 88 0
97 G 187-8 WD* 20 50 20.6528403623 +26 30 40.767339538       15.30   DA9 55 0
98 Ross 193B WD* 20 56 47.7846012257 -04 50 39.537436123   17.81 16.68     DC10 75 0
99 LAWD 83 WD* 21 13 16.8549349741 -81 49 12.878285501 13.28 13.82 13.59 13.6   DA4.8 125 0
100 EGGR 378 WD* 21 18 56.2636115928 +54 12 41.243943888 11.76     12.9   DA3.4 111 1
101 EGGR 148 WD* 21 42 41.0063054408 +20 59 58.123903616   13.40   12.9   DQ6 128 0
102 WG 39 WD* 21 57 38.3567715267 -51 00 31.521044535   14.94 14.73 14.53   DQ7 87 0
103 EGGR 155 WD* 22 49 05.5507896558 +22 36 31.991540832   14.55   13.8   DA4.7 111 0
104 LP 761-114 WD* 22 51 55.4101964976 -10 15 02.880938952   17.1 17.45 11.9   DA 20 0
105 EGGR 453 WD* 22 53 53.3851734316 -06 46 54.488228178   17.53 15.66 15.70   DZ13 104 1
106 V* ZZ Psc WD* 23 28 47.6365087803 +05 14 54.235051503   13.217   13.106   DA4.1 536 0
107 GD 1212 WD* 23 38 50.7400887024 -07 41 19.970752560   13.44 13.26   13.24 DA4.5 64 0
108 LAWD 93 WD* 23 43 50.7212145360 +32 32 46.728318300   13.06 12.94 13.12   DA3.8 160 0
109 LAWD 94 WD* 23 54 01.0726392457 -33 16 31.078214643   14.6 13.56     DA5.7 63 0

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