2018A&A...617A..83V


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.04CEST14:01:16

2018A&A...617A..83V - Astronomy and Astrophysics, volume 617A, 83-83 (2018/9-1)

VLTI/MIDI atlas of disks around low- and intermediate-mass young stellar objects.

VARGA J., ABRAHAM P., CHEN L., RATZKA T., GABANYI K.E., KOSPAL A., MATTER A., VAN BOEKEL R., HENNING T., JAFFE W., JUHASZ A., LOPEZ B., MENU J., MOOR A., MOSONI L. and SIPOS N.

Abstract (from CDS):


Context. Protoplanetary disks show large diversity regarding their morphology and dust composition. With mid-infrared interferometry the thermal emission of disks can be spatially resolved, and the distribution and properties of the dust within can be studied.
Aims. Our aim is to perform a statistical analysis on a large sample of 82 disks around low- and intermediate-mass young stars, based on mid-infrared interferometric observations. We intend to study the distribution of disk sizes, variability, and the silicate dust mineralogy.
Methods. Archival mid-infrared interferometric data from the MIDI instrument on the Very Large Telescope Interferometer are homogeneously reduced and calibrated. Geometric disk models are used to fit the observations to get spatial information about the disks. An automatic spectral decomposition pipeline is applied to analyze the shape of the silicate feature.
Results. We present the resulting data products in the form of an atlas, containing N band correlated and total spectra, visibilities, and differential phases. The majority of our data can be well fitted with a continuous disk model, except for a few objects, where a gapped model gives a better match. From the mid-infrared size-luminosity relation we find that disks around T Tauri stars are generally colder and more extended with respect to the stellar luminosity than disks around Herbig Ae stars. We find that in the innermost part of the disks (r~=1au) the silicate feature is generally weaker than in the outer parts, suggesting that in the inner parts the dust is substantially more processed. We analyze stellar multiplicity and find that in two systems (AB Aur and HD 72106) data suggest a new companion or asymmetric inner disk structure. We make predictions for the observability of our objects with the upcoming Multi-AperTure mid-Infrared SpectroScopic Experiment (MATISSE) instrument, supporting the practical preparations of future MATISSE observations of T Tauri stars.

Abstract Copyright: © ESO 2018

Journal keyword(s): protoplanetary disks - stars: pre-main sequence - techniques: interferometric - circumstellar matter - infrared: stars

VizieR on-line data: <Available at CDS (J/A+A/617/A83): table1.dat table2.dat tablee1.dat refs.dat fits/*>

Simbad objects: 90

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Number of rows : 90

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 [RAC97] VLA 4b Rad 03 29 03.740 +31 16 04.15           ~ 19 0
2 V* V512 Per Or* 03 29 03.7567945196 +31 16 03.959183877           ~ 348 0
3 EM* LkHA 330 TT* 03 45 48.2804487421 +32 24 11.851014679   12.30 10.97     F7 121 0
4 V* RY Tau Or* 04 21 57.4132838427 +28 26 35.533990877 10.82 10.34 9.30 9.67 8.87 K1IV/Ve 648 1
5 NAME T Tau S ** 04 21 59.371 +19 32 05.95           K7 139 2
6 NAME T Tau Sb *i* 04 21 59.371 +19 32 05.95           M1 70 0
7 NAME T Tau Sa *i* 04 21 59.371 +19 32 05.95           ~ 65 0
8 V* T Tau Or* 04 21 59.4323326335 +19 32 06.439974179   11.01 9.30 9.80   K0IV/Ve 1249 2
9 NAME T Tau N *i* 04 21 59.433 +19 32 06.42   11.22 10.12 9.80   K1.5 164 1
10 V* DG Tau Or* 04 27 04.6913654419 +26 06 16.041555299 13.57 13.97 10.50 12.28   K6Ve 923 1
11 V* GV Tau B * 04 29 23.68680 +24 33 01.1160           ~ 27 0
12 V* GV Tau A * 04 29 23.71056 +24 32 58.6176           ~ 23 0
13 V* GV Tau TT* 04 29 23.7314759229 +24 33 00.216016292 19.20         K7 271 2
14 RAFGL 5123 FU* 04 31 34.07736 +18 08 04.9020           K3V/M3III 811 0
15 V* HL Tau Or* 04 31 38.471952 +18 13 58.08504   15.89 14.49 14.39   K5 1201 0
16 V* GG Tau Or* 04 32 30.3318954228 +17 31 40.834888327 14.84 14.78 13.40 11.54   M0e+M2.0e 647 1
17 EM* LkCa 15 Or* 04 39 17.7912813350 +22 21 03.387667491   13.01 12.03 11.61   K5:Ve 552 1
18 V* DR Tau Or* 04 47 06.2152696011 +16 58 42.814250257 12.03 11.86 10.50 12.19   K5Ve 467 0
19 V* UY Aur Or* 04 51 47.3900418279 +30 47 13.552212742 12.82 12.96 11.90 10.59 9.52 M0e+M2.5e 326 0
20 V* GM Aur Or* 04 55 10.9813656049 +30 21 59.375978047 14.59 14.22 13.10     K3Ve 552 0
21 V* AB Aur Ae* 04 55 45.8459978418 +30 33 04.293281305 7.20 7.16 7.05 6.96 6.70 A0Ve 930 2
22 V* SU Aur Or* 04 55 59.3861369488 +30 34 01.499800471   10.33 9.30 9.17   G2IIIne 532 0
23 HD 31648 Ae* 04 58 46.2654165113 +29 50 36.990341242 7.84 7.78 7.62 7.76 7.43 A5Vep 394 0
24 V* UX Ori Ae* 05 04 29.9881676817 -03 47 14.288047238 10.25 10.93 8.70 9.62 9.43 A4IVe 333 1
25 V* CO Ori Or* 05 27 38.3352 +11 25 38.923 12.96 12.33 10.30 10.33 9.63 F7Ve 155 0
26 V* GW Ori Or* 05 29 08.3925564419 +11 52 12.653756566   10.83 10.10 9.52   G5/8Ve 299 0
27 HD 36112 Ae* 05 30 27.5286772598 +25 19 57.082162439   8.57 8.27     A8Ve 358 0
28 V* NY Ori Or* 05 35 36.0089313187 -05 12 25.294778566 14.079 13.847 13.232   11.445 G6-K2e 60 0
29 V* CQ Tau Ae* 05 35 58.4671238887 +24 44 54.086375712 11.290 10.780 10.000   8.33 F5IVe 255 0
30 V* V1247 Ori dS* 05 38 05.2518310146 -01 15 21.696624736   10.18 9.82     F0V 73 0
31 V* V883 Ori Or* 05 38 18.0974260202 -07 02 25.963144400   14.80       F:I: 107 0
32 HD 37806 Be* 05 41 02.2930276072 -02 43 00.729083804 7.67 7.93 7.90     B9/9.5II/III 138 0
33 V* FU Ori Or* 05 45 22.3650208559 +09 04 12.296285806   10.72 9.60     F0Iab 708 1
34 V* V1647 Ori Or* 05 46 13.1370923766 -00 06 04.876812846     18.1     ~ 231 1
35 V* V900 Mon Or* 06 57 22.2228213858 -08 23 17.681793444   15.94 14.71     ~ 22 0
36 V* Z CMa Ae* 07 03 43.1588002461 -11 33 06.230351311 10.51 9.99 8.80     B5/8eq+F5/7 532 3
37 V* V646 Pup Or* 07 50 35.5923632458 -33 06 23.904713538   13.96 12.65 12.04   ~ 62 0
38 HD 72106 ** 08 29 34.89852 -38 36 21.1321       9.32   A0IV 61 0
39 Hen 3-545 Or* 10 59 06.9712894449 -77 01 40.309036535   12.91 11.136   9.596 K4Ve 188 0
40 V* TW Hya TT* 11 01 51.9054298616 -34 42 17.031550898   11.94 10.50 10.626 9.18 K6Ve 1532 1
41 V* DI Cha Or* 11 07 20.7272524388 -77 38 07.303742740   12.02 10.74 10.72   G2Ve 145 0
42 V* HP Cha B * 11 08 14.7682489051 -77 33 52.732866898           G5e 15 0
43 V* HP Cha Or* 11 08 15.216432 -77 33 53.17020   14.33 12.77 12.11   K3+G5e 99 0
44 V* HP Cha A * 11 08 15.4942983813 -77 33 53.454218639           K6e 80 0
45 Ass Cha T 1-23 Or* 11 09 53.4191770981 -76 34 25.652662545   13.9 19.50 15.10 13.52 G9IIIe 80 0
46 V* WW Cha Or* 11 10 00.0791962314 -76 34 57.971855660   14.74 14.10   10.95 ~ 130 0
47 V* CV Cha Or* 11 12 27.7052551478 -76 44 22.298597430   12.02 10.98 10.51 9.76 G9Ve 171 1
48 HD 100546 Be* 11 33 25.4404858122 -70 11 41.239343121   6.71 6.30   6.64 A0VaekB8_lB 651 1
49 HD 101412 Be* 11 39 44.4562795603 -60 10 27.717502041   9.465 9.288     A3VaekA0mA0_lB 115 0
50 V* DX Cha Ae* 12 00 05.0870448691 -78 11 34.559255151   6.81 6.60     A0_sh 306 0
51 V* DK Cha Or* 12 53 17.2028372976 -77 07 10.727661977           F0 132 0
52 CPD-36 6759 Y*O 15 15 48.4459023859 -37 09 16.026315179   9.21 8.708     F8V 357 1
53 HD 135344 * 15 15 48.9457954324 -37 08 55.727525343   7.84 7.76     A0V 128 1
54 HD 139614 pr* 15 40 46.3818973118 -42 29 53.538928508   8.47 8.24     A9VekA5mA5(_lB) 160 0
55 HD 141569 pr* 15 49 57.7484743862 -03 55 16.344023102 7.22 7.20 7.12 7.00 7.04 A2VekB9mB9(_lB) 470 0
56 HD 142666 TT* 15 56 40.0222941557 -22 01 40.004849949 9.41 9.37 8.82 8.31 8.01 F0V_sh 217 0
57 HD 142527 Ae* 15 56 41.8888096574 -42 19 23.245384377   9.04 8.34     F6III 467 1
58 HD 142527b Pl? 15 56 41.8888096574 -42 19 23.245384377           ~ 17 0
59 V* RU Lup Or* 15 56 42.3109948086 -37 49 15.473469159 9.27 10.07 9.60     K7/M0e 382 0
60 HD 143006 Or* 15 58 36.9127773803 -22 57 15.221492622   10.92 10.14   8.70 G5IVe 166 0
61 HD 325367 Or* 16 03 05.4914377137 -40 18 25.426543472   11.40 8.50     M0 276 0
62 HD 144132 * 16 04 12.7125378065 +02 46 49.456520399   9.94 8.73     K2III 6 0
63 HD 144432 Ae* 16 06 57.9530266912 -27 43 09.758016578 8.47 8.53 8.19 7.82 7.53 A9/F0V 211 1
64 V* V856 Sco Ae* 16 08 34.2868591379 -39 06 18.326059778 7.66 7.41 7.05 6.92   A7IIIne_sh 351 0
65 V* V866 Sco Or* 16 11 31.345632 -18 38 25.96200   13.98 12.63 12.81   K0e+K5e 244 0
66 EM* SR 4 Or* 16 25 56.1659484606 -24 20 48.239269835     12.80 11.7 10.7 K0:Ve 151 1
67 Haro 1-6 Or* 16 26 03.0281201323 -24 23 36.193999164   14.15 14.01 12.38 10.80 K0 204 1
68 GSS 31 TT* 16 26 23.3694945462 -24 20 59.580653864   15.9 14.70 14.33 11.53 K0e 133 1
69 DoAr 25 TT* 16 26 23.6911216715 -24 43 13.886717283       12.65   K5 128 0
70 EM* SR 24B TT* 16 26 58.4363490468 -24 45 32.211217104           M0.5e 78 0
71 EM* SR 24A TT* 16 26 58.5027167089 -24 45 36.698300286       14.15 12.87 K1 91 0
72 EM* SR 21A TT* 16 27 10.2776332501 -24 19 12.620553212   16.08 14.10     G1 233 1
73 YLW 13B Y*O 16 27 21.46872 -24 41 43.0692           ~ 86 0
74 IRAS 16245-2423 TT* 16 27 37.1911764648 -24 30 35.031583716       16.66 14.67 B5-F2 235 0
75 EM* SR 9 Or* 16 27 40.2858402419 -24 22 04.132012501   12.91 11.533 11.11 10.00 K5e 249 0
76 Haro 1-16 Or* 16 31 33.4638378966 -24 27 37.158295501   14.02 12.80     K3e 175 0
77 IRAS 16289-4449 Or* 16 32 32.19264 -44 55 30.6552       15.95   ~ 116 1
78 HD 150193B TT* 16 40 17.865 -23 53 45.95           ~ 11 0
79 HD 150193A Ae* 16 40 17.923 -23 53 45.17   9.39 8.88     ~ 6 0
80 HD 150193 Be* 16 40 17.9242900066 -23 53 45.192676418 9.69 9.32 8.79 8.41   B9.5Ve 290 0
81 EM* AS 209 Or* 16 49 15.3035547820 -14 22 08.642015783   12.62 11.28     K4Ve 233 0
82 V* AK Sco Ae* 16 54 44.8497760618 -36 53 18.560813962 9.80 9.63 9.00     F5V 235 1
83 HD 163296 Ae* 17 56 21.2882188601 -21 57 21.872343282 7.00 6.93 6.85 6.86 6.67 A1Vep 802 0
84 HD 169142 Ae* 18 24 29.7799676975 -29 46 49.328597698   8.42 8.16     F1VekA3mA3_lB? 335 2
85 V* VV Ser Ae* 18 28 47.8619658319 +00 08 39.924642619 12.99 12.63 11.80 11.01 10.24 A5Ve 228 0
86 IRAS 18274+0112 Y*O 18 29 57.73680 +01 14 05.6940           M4: 135 2
87 V* S CrA Or* 19 01 08.597088 -36 57 19.89504   11.76 10.91 11.41   G0Ve+K0Ve 258 0
88 V* T CrA Ae* 19 01 58.7901571143 -36 57 50.329832417     11.67     F0 155 0
89 V* VV CrA Or* 19 03 06.7419790029 -37 12 49.683383133   16.45 14.67 14.12 11.62 K7 107 0
90 HD 179218 Ae* 19 11 11.2540715594 +15 47 15.632212730 7.55 7.476 7.39 7.25 7.21 A0Ve 220 0

    Equat.    Gal    SGal    Ecl

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2020.07.04-14:01:16

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