2011ApJ...726...30M


Query : 2011ApJ...726...30M

2011ApJ...726...30M - Astrophys. J., 726, 30 (2011/January-1)

The first ultra-cool brown dwarf discovered by the Wide-field Infrared Survey Explorer.

MAINZER A., CUSHING M.C., SKRUTSKIE M., GELINO C.R., KIRKPATRICK J.D., JARRETT T., MASCI F., MARLEY M.S., SAUMON D., WRIGHT E., BEATON R., DIETRICH M., EISENHARDT P., GARNAVICH P., KUHN O., LEISAWITZ D., MARSH K., McLEAN I., PADGETT D. and RUEFF K.

Abstract (from CDS):

We report the discovery of the first new ultra-cool brown dwarf (BDs) found with the Wide-field Infrared Survey Explorer (WISE). The object's preliminary designation is WISEPC J045853.90+643451.9. Follow-up spectroscopy with the LUCIFER instrument on the Large Binocular Telescope indicates that it is a very late-type T dwarf with a spectral type approximately equal to T9. Fits to an IRTF/SpeX 0.8-2.5 µm spectrum to the model atmospheres of Marley and Saumon indicate an effective temperature of approximately 600 K as well as the presence of vertical mixing in its atmosphere. The new BD is easily detected by WISE, with a signal-to-noise ratio of ∼36 at 4.6 µm. Current estimates place it at a distance of 6-10 pc. This object represents the first in what will likely be hundreds of nearby BDs found by WISE that will be suitable for follow-up observations, including those with the James Webb Space Telescope. One of the two primary scientific goals of the WISE mission is to find the coolest, closest stars to our Sun; the discovery of this new BD proves that WISE is capable of fulfilling this objective.

Abstract Copyright:

Journal keyword(s): brown dwarfs - infrared: stars - solar neighborhood - stars: late-type - stars: low-mass

Simbad objects: 19

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Number of rows : 19
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 CFBDS J003402-005206 BD* 00 34 02.77416 -00 52 06.8196           T8+/Y? 49 0
2 CFBDS J005910-011401 BD* 00 59 10.46265 -01 14 00.5404           T9.0 38 0
3 SIMP J013656.5+093347.3 BD* 01 36 56.5605419830 +09 33 47.311965969           T2.0 128 0
4 HD 14632 SB* 02 24 17.7290846664 +63 02 31.993454400   7.766 7.633     A0V 20 0
5 2MASSI J0415195-093506 BD* 04 15 19.54368 -09 35 06.6732           T8.0 165 0
6 2MASS J04510093-3402150 BD* 04 51 00.9451841616 -34 02 14.908896132           L0.5 21 0
7 WISE J045853.89+643452.5 BD* 04 58 53.89392 +64 34 52.5900           T8.5 25 0
8 HD 33541 SB* 05 18 13.2421269840 +73 16 05.150872740 5.670 5.790 5.830     A0V 36 0
9 WISE J072227.27-054029.9 BD* 07 22 27.51096 -05 40 31.2096           T9 75 0
10 2MASS J08354256-0819237 BD* 08 35 42.5314423948 -08 19 23.372129099           L6.5 67 0
11 SDSS J083717.21-000018.0 BD* 08 37 17.20032 -00 00 19.3608           T1 51 0
12 ULAS J133553.45+113005.2 BD* 13 35 53.45352 +11 30 05.1444           T8+/Y? 38 0
13 ULAS J141623.94+134836.3 BD* 14 16 23.94216 +13 48 36.3204           T7.5p 56 0
14 NAME Proxima Centauri Er* 14 29 42.9461331854 -62 40 46.164680672 14.21 12.95 11.13 9.45 7.41 M5.5Ve 1299 0
15 GJ 570 D BD* 14 57 14.96256 -21 21 47.7504           T8 225 1
16 2MASSI J1546271-332511 BD* 15 46 27.18600 -33 25 11.1828           T5.7 31 1
17 2MASS J16241436+0029158 BD* 16 24 14.36712 +00 29 15.8172           T6V 145 0
18 2MASS J16322911+1904407 BD* 16 32 29.11416 +19 04 40.7136       22.42 19.98 L8V 131 0
19 Wolf 940 B BD* 21 46 38.829 -00 10 38.59           T8+/Y? 57 0

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