2010ApJ...710L..26K


Query : 2010ApJ...710L..26K

2010ApJ...710L..26K - Astrophys. J., 710, L26-L29 (2010/February-2)

New debris disk candidates around 49 nearby stars.

KOERNER D.W., KIM S., TRILLING D.E., LARSON H., COTERA A., STAPELFELDT K.R., WAHHAJ Z., FAJARDO-ACOSTA S., PADGETT D. and BACKMAN D.

Abstract (from CDS):

We present 49 new candidate debris disks that were detected around nearby stars with the Spitzer Space Telescope using the Multiband Imaging Photometer (MIPS) at 24 µm (MIPS24) and 70 µm (MIPS70). The survey sample was composed of stars within 25 pc of the Sun that were not previously observed by any other MIPS survey. Only stars with V < 9 were selected, corresponding to spectral types earlier than M0. MIPS24 integration times were chosen to detect the stellar photosphere at 10σ levels or better. MIPS70 observations were designed to detect excess infrared emission from any star in the MIPS70 sample with a disk as luminous at that around ε Eridani. The resulting sample included over 436 nearby stars that were observed with both MIPS24 and MIPS70, plus an additional 198 observed only with MIPS24. Debris disk candidates were defined as targets where excess emission was detected at 3σ levels or greater, and the ratio of observed flux density to expected photosphere emission was three standard deviations or more above the mean value for the sample. The detection rate implied by the resulting 29 MIPS24 candidates is 4.6%. A detection rate of 4.8% is implied by 21 MIPS70 candidates. The distribution of spectral types for stars identified as candidates resembles that of the general sample and yields strong evidence that debris-disk occurrence does not decrease for K dwarfs. Modeling of non-uniform sensitivity in the sample is required to interpret quantitative estimates of the overall detection frequency and will be presented in a future work.

Abstract Copyright: ∼

Journal keyword(s): circumstellar matter - infrared: stars - protoplanetary disks - solar neighborhood

Simbad objects: 51

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Number of rows : 51
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 HD 224953 ** 00 02 08.73610 -68 16 50.7519 11.838 10.646 9.241 8.372 7.533 K5/M0V 33 0
2 * 85 Peg SB* 00 02 10.3487193861 +27 04 54.599101714 6.47 6.42 5.75 5.16 4.73 G5VbFe-2 568 0
3 BD+40 45 PM* 00 17 06.3740983357 +40 56 53.870823378   10.36   8.2   K7V 138 0
4 HD 1461 PM* 00 18 41.8676757921 -08 03 10.803829898   7.14 6.46     G3VFe0.5 413 1
5 HD 1562 PM* 00 20 00.4079121242 +38 13 38.631661719   7.61   6.6   G1V 94 0
6 HD 4378 ** 00 45 48.28710 -41 54 33.0961 10.358 9.144 7.881 7.115 6.466 K5/M0V 45 0
7 HD 4378A PM* 00 45 48.2871509825 -41 54 33.080290572   9.58 8.37     K5Ve 31 0
8 * 64 Psc SB* 00 48 58.7075574408 +16 56 26.324381004   5.58   4.8   F8V 149 0
9 HD 5133 PM* 00 53 01.1348555154 -30 21 24.891057111 8.801 8.11 7.171 6.639 6.179 K2.5Vk: 186 0
10 * mu. Cas SB* 01 08 16.3029454473 +54 55 12.561201263 5.93 5.86 5.17 4.55 4.13 G5Vb 593 1
11 * chi Cet PM* 01 49 35.1027660619 -10 41 11.070999501 5.04 5.00 4.68 4.38 4.22 F0V 215 0
12 * 12 Per SB* 02 42 14.9145674304 +40 11 38.221732500 5.65 5.51 4.92 4.42 4.12 F9V 193 0
13 HD 18143A PM* 02 55 39.0594192621 +26 52 23.574873795   8.73 7.68     K2IV 146 0
14 * eps Eri BY* 03 32 55.8444911587 -09 27 29.739493865 5.19 4.61 3.73 3.00 2.54 K2V 2073 1
15 HD 23484 PM* 03 44 09.1729719544 -38 16 54.372263223 8.449 7.875 6.996 6.516 6.09 K2V 136 0
16 G 221-24 ** 03 48 01.6922324912 +68 40 38.765916556   12.28 10.81 10.15   M2V+K6V 65 0
17 * gam Dor gD* 04 16 01.5866224848 -51 29 11.932714356   4.55 4.20     F1V 337 0
18 * alf Cae PM* 04 40 33.7125133631 -41 51 49.504549835 4.79 4.79 4.45 4.11 3.90 F2V 134 0
19 HD 34751 PM* 05 18 47.1904685616 -21 23 37.524706188 11.903 11.08 9.52     K6Vk 67 0
20 V* VZ Col BY? 05 30 14.0042313744 -42 41 50.379896724 12.333 11.096 9.706 8.851 8.078 M0V 39 0
21 HD 45184 PM* 06 24 43.8795895848 -28 46 48.415725948   7.01 6.39 6.24 8.94 G2Va 238 1
22 HD 49601 PM* 06 51 32.3938070547 +47 22 04.146058752   10.21   8.2   K6V 77 0
23 HD 60491 BY* 07 34 26.1676173360 -06 53 48.036803172 9.554 9.027 8.144 7.654 7.214 K1V 99 0
24 BD+66 582 PM* 08 52 00.3480148704 +66 07 53.387584968   10.63 9.28     K5V 68 0
25 HD 77175A PM* 09 01 17.4768597774 +15 15 56.754817933   10.53 9.34 9.07   K6V 62 0
26 * 39 Leo PM* 10 17 14.5383472150 +23 06 22.384190401 6.27 6.32 5.82 5.34 5.07 F6V 219 0
27 HD 97584 PM* 11 15 11.9031954572 +73 28 30.737755312   8.70 7.65 8.09   K4V 95 0
28 HD 103932 PM* 11 57 56.2063477236 -27 42 25.366588848 9.23 8.114 6.964 6.298 5.758 K4+V 178 0
29 HD 104067 PM* 11 59 10.0088449029 -20 21 13.612067116 9.683 8.897 7.921 7.369 6.913 K2V 149 1
30 HD 104304 SB* 12 00 44.4601479291 -10 26 46.067117528 6.76 6.32 5.55     G8IV 264 0
31 HD 119332 PM* 13 41 13.4048636208 +56 43 37.821650160   8.62 7.78     K0IV-V 58 0
32 BD+39 2801 PM* 14 48 01.4253727008 +38 27 58.440538008   11.16 9.711 9.349   K7Ve 58 0
33 V* DE Boo RS* 14 53 23.7654730144 +19 09 10.072718521   6.84 6.00 5.5   K0.5V 287 0
34 HD 132899 ** 15 03 06.11633 -41 59 33.2128 11.179 10.123 8.960 8.255 7.612 K4.5Vk: 24 0
35 * 5 Ser PM* 15 19 18.7974409923 +01 45 55.466382064   5.60   4.8   F8IV 355 0
36 * bet TrA PM* 15 55 08.5620636 -63 25 50.615531 3.19 3.14 2.85 2.53 2.38 F1V 174 0
37 CD-32 11389 PM* 16 04 23.1464872371 -33 03 39.692935532 12.682 11.45 10.075 9.215 8.405 K8Vk 30 0
38 * 49 Ser A ** 16 13 18.4497126173 +13 31 36.845416252   8.12 7.34     G9V 124 0
39 HD 153026 ** 16 58 54.05078 -39 33 30.7785 10.597 9.497 8.320 7.602 6.963 K4.5Vk: 27 0
40 HD 158233 PM* 17 29 06.5560515696 -23 50 10.003726320 12.053 10.904 9.597 8.798 8.111 K5V 44 0
41 BD+23 3151A PM* 17 37 48.7002864168 +22 57 20.090682360   11.20 9.93 9.1   M0.5V 61 0
42 * b Her SB* 18 07 01.5906608928 +30 33 43.584892488 5.52 5.67 5.13 4.61 4.28 F6V 493 0
43 HD 191499 ** 20 09 34.30429 +16 48 20.7457 8.825 8.372 7.515 7.033 6.571 G9V 48 0
44 HD 340345 ** 20 30 10.6682708731 +26 50 34.200586250       9.303   M1V 59 0
45 * eps Cyg ** 20 46 12.6722768426 +33 58 13.182037125 4.370 3.520 2.480 1.73 1.19 K0III 519 0
46 HD 200968 PM* 21 07 10.3811555132 -13 55 22.528267753 8.578 8.10 7.19 6.581 6.101 K1IV 114 0
47 HD 202628 PM* 21 18 27.2696247000 -43 20 04.743062448   7.39 6.742     G5V 208 0
48 HD 208038 PM* 21 53 05.3532467280 +20 55 49.871111232 9.734 9.078 8.148 7.638 7.18 K2.5V 78 0
49 HD 215152 PM* 22 43 21.3028100652 -06 24 02.953048623   9.12 8.13 7.83 8.46 K3V 141 1
50 HD 223778 SB* 23 52 25.4091266714 +75 32 40.354906472   7.35 6.38 5.8   K3V 143 0
51 BD+28 4660 PM* 23 53 08.5915230024 +29 01 05.036070036   11.2 9.830 9.319   K6V 56 0

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