SIMBAD references

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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2020.10.25-10:01:20

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