2015MNRAS.449.2472B


Query : 2015MNRAS.449.2472B

2015MNRAS.449.2472B - Mon. Not. R. Astron. Soc., 449, 2472-2488 (2015/May-3)

The JCMT Gould Belt Survey: SCUBA-2 observations of circumstellar discs in L 1495.

BUCKLE J.V., DRABEK-MAUNDER E., GREAVES J., RICHER J.S., MATTHEWS B.C., JOHNSTONE D., KIRK H., BEAULIEU S.F., BERRY D.S., BROEKHOVEN-FIENE H., CURRIE M.J., FICH M., HATCHELL J., JENNESS T., MOTTRAM J.C., NUTTER D., PATTLE K., PINEDA J.E., SALJI C., TISI S., DI FRANCESCO J., HOGERHEIJDE M.R., WARD-THOMPSON D., BASTIEN P., BUTNER H., CHEN M., CHRYSOSTOMOU A., COUDE S., DAVIS C.J., DUARTE-CABRAL A., FRIBERG P., FRIESEN R., FULLER G.A., GRAVES S., GREGSON J., HOLLAND W., JONCAS G., KIRK J.M., KNEE L.B.G., MAIRS S., MARSH K., MORIARTY-SCHIEVEN G., RAWLINGS J., ROSOLOWSKY E., RUMBLE D., SADAVOY S., THOMAS H., TOTHILL N., VITI S., WHITE G.J., WILSON C.D., WOUTERLOOT J., YATES J. and ZHU M.

Abstract (from CDS):

We present 850 and 450 µm data from the James Clerk Maxwell Telescope (JCMT) Gould Belt Survey obtained with Submillimetre Common-User Bolometer Array 2 (SCUBA-2) and characterize the dust attributes of Class I, Class II and Class III disc sources in L 1495. We detect 23 percent of the sample at both wavelengths, with the detection rate decreasing through the Classes from I to III. The median disc mask is 1.6x10–3 M☉, and only 7 percent of Class II sources have disc masses larger than 20 Jupiter masses. We detect a higher proportion of discs towards sources with stellar hosts of spectral type K than spectral type M. Class II discs with single stellar hosts of spectral type K have higher masses than those of spectral type M, supporting the hypothesis that higher mass stars have more massive discs. Variations in disc masses calculated at the two wavelengths suggest that there may be differences in dust opacity and/or dust temperature between discs with hosts of spectral types K to those with spectral type M.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): stars: formation - stars: low mass - submillimetre: ISM

Simbad objects: 60

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Number of rows : 60
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 V* V1095 Tau TT* 04 13 14.1551534304 +28 19 10.668859500   15.32 13.81 13.62   M4 123 0
2 V* V1096 Tau TT* 04 13 27.2218223808 +28 16 24.656012868   15.42 13.53 13.07   M0 93 0
3 NAME IRAS 04108+2803A Or* 04 13 53.2833187728 +28 11 23.218994688           M5.5 39 0
4 NAME IRAS 04108+2803B Y*O 04 13 54.71688 +28 11 32.8992           K0-M3 45 0
5 2MASS J04141188+2811535 Or* 04 14 11.8840810320 +28 11 53.409534000 18.72         M6e 68 0
6 IRAS F04110+2800 Y*O 04 14 12.28944 +28 08 37.1724           ~ 28 0
7 HD 283447 Or* 04 14 12.9261150912 +28 12 12.359055168 13.17 12.07 10.68 9.45 8.67 K3Ve 445 0
8 V* FM Tau Or* 04 14 13.5841955640 +28 12 49.168982592 14.44   13.80 13.64   M0/2e 227 0
9 V* FN Tau TT* 04 14 14.5945463760 +28 27 58.067731188     14.70 13.68   M5e 178 0
10 V* CW Tau TT* 04 14 17.0042670144 +28 10 57.766508508 13.92 13.64 12.36 12.86   K0Ve 381 0
11 [BCG93] 1 TT* 04 14 17.6095515480 +28 06 09.654704388 18.04         M4.5 126 0
12 [BHS98] MHO 1 TT* 04 14 26.2681279416 +28 06 03.270677040           ~ 49 1
13 [BHS98] MHO 2 TT* 04 14 26.4009435600 +28 05 59.635905324           M2.5 64 1
14 NAME IRAS 04114+2757G TT* 04 14 30.5508810936 +28 05 14.596567332           M2.2 61 0
15 2MASS J04144158+2809583 BD* 04 14 41.58936 +28 09 58.3236           L2.3 11 0
16 2MASS J04144739+2803055 TT* 04 14 47.3955097368 +28 03 05.518180080           M5.2 38 0
17 V* FO Tau Or* 04 14 49.2843205392 +28 12 30.505096476       14.92   M3.5e+M3.5e 139 0
18 UCAC4 591-011866 TT* 04 14 52.310472 +28 05 59.69616 19.87         M3.1 31 0
19 [BCG93] 2 TT* 04 15 05.1562986720 +28 08 46.055825016           M5.5 54 0
20 [BLH2002] KPNO-Tau 1 LM* 04 15 14.7215444352 +28 00 09.383811048     24.063     M8.5Ve 44 0
21 2MASS J04153566+2847417 Or* 04 15 35.6823994296 +28 47 41.349234984           M6.3 15 0
22 2MASS J04153916+2818586 TT* 04 15 39.1632520536 +28 18 58.525247124           M4.0 52 0
23 2MASS J04155799+2746175 TT* 04 15 57.9994267200 +27 46 17.332228344           M5.2 50 0
24 2MASS J04161210+2756385 Or* 04 16 12.1079972592 +27 56 38.479557732           M5e 48 0
25 2MASS J04161726+2817128 Or* 04 16 17.2626408312 +28 17 12.814874196           M4.75 27 0
26 2MASS J04161885+2752155 TT* 04 16 18.8582426064 +27 52 15.368261376           M8.0 38 0
27 EM* LkCa 4 Or* 04 16 28.1067298272 +28 07 35.731363080   13.96 12.78 11.825   K7:Ve 208 0
28 2MASS J04163911+2858491 TT* 04 16 39.1233968760 +28 58 49.329653232           M7.3 38 0
29 V* CY Tau Or* 04 17 33.7284990744 +28 20 46.812121656 14.52 14.68 13.40 12.59   M1.5 297 0
30 V* V1312 Tau TT* 04 17 38.9450182296 +28 33 00.578450700   15.57 13.26 13.12   M2 113 0
31 [BLH2002] KPNO-Tau 10 Or* 04 17 49.5567002040 +28 13 31.770031152     17.8     M5Ve 57 0
32 IRAS F04147+2822 TT* 04 17 49.6577031384 +28 29 36.318234912           M3.7 89 0
33 LDN 1495 DNe 04 18.1 +27 37           ~ 408 1
34 [SS94] V410 X-ray 3 TT* 04 18 07.9729489560 +28 26 03.667161660     18.319     M6 82 0
35 2MASS J04181710+2828419 TT* 04 18 17.1069408984 +28 28 41.928528396     22.175     M6.4 93 0
36 2MASS J04182909+2826191 Y*O 04 18 29.09760 +28 26 19.1148           ~ 37 0
37 [BLH2002] KPNO-Tau 11 TT* 04 18 30.3020636616 +27 43 20.654543028           M5.5Ve 52 0
38 V* V410 Tau Or* 04 18 31.1081296680 +28 27 16.155955728   12.13 10.75 8.45 9.408 K3Ve 483 0
39 V* DD Tau Or* 04 18 31.1289436392 +28 16 29.148496644 15.94 15.49 14.10 13.76   M3.5e+M3.5e 209 0
40 SSTtau 041831.2+282617 Y*O 04 18 31.23168 +28 26 18.0492           ~ 11 0
41 V* CZ Tau Or* 04 18 31.5898864272 +28 16 58.150241544 15.96 16.60 15.70 14.77   M2 149 0
42 IRAS 04154+2823 Or* 04 18 32.0443900008 +28 31 14.971419300           M2.5 69 0
43 2MASS J04183444+2830302 Y*O 04 18 34.44696 +28 30 30.2256           M0 48 0
44 2MASS J04184023+2824245 TT* 04 18 40.2362238576 +28 24 24.058269540           ~ 40 0
45 V* V892 Tau Ae* 04 18 40.6157618376 +28 19 15.625058880   16.6 14.69 14.35   A0Ve 324 0
46 LR 1 Y*O 04 18 41.33232 +28 27 25.0092           K7 42 0
47 [SS94] V410 X-ray 7 TT* 04 18 42.5008529280 +28 18 49.922715996       18.02 15.42 M0.5e 47 0
48 V* V1023 Tau Or* 04 18 47.0291197872 +28 20 07.493080560   14.31 12.00 11.21   K7 178 0
49 [BLH2002] KPNO-Tau 2 LM* 04 18 51.1523690496 +28 14 33.297388728     21.376     M7.5Ve 50 0
50 NAME CoKu Tau 1 Y*O 04 18 51.4683860880 +28 20 26.373956172     19.3     K7+M 88 0
51 IRAS 04158+2805 Or* 04 18 58.1336295120 +28 12 23.355499140           M5.25 124 0
52 2MASS J04190110+2819420 TT* 04 19 01.1052204768 +28 19 42.090142476           M5.9 77 0
53 [BLH2002] KPNO-Tau 12 Or* 04 19 01.2829227024 +28 02 48.139594656     23.228     M9Ve 57 0
54 2MASS J04190197+2822332 TT* 04 19 01.9772015400 +28 22 33.269537064           M5.5 53 0
55 V* FQ Tau Or* 04 19 12.812616 +28 29 32.98128       15.00   M3 117 0
56 WK81 1 TT* 04 19 26.2675117776 +28 26 14.259575472   14.81 13.04 12.240   K7 249 1
57 V* FR Tau Or* 04 19 35.4592547640 +28 27 21.878830512       16.22   M5.3 69 0
58 2MASS J04201611+2821325 Or* 04 20 16.1147942712 +28 21 32.516976168           M8.3 40 0
59 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
60 NAME Gould Belt PoG ~ ~           ~ 956 1

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