2015ApJ...811..145J


Query : 2015ApJ...811..145J

2015ApJ...811..145J - Astrophys. J., 811, 145 (2015/October-1)

The dustiest post-main sequence stars in the Magellanic Clouds.

JONES O.C., MEIXNER M., SARGENT B.A., BOYER M.L., SEWILO M., HONY S. and ROMAN-DUVAL J.

Abstract (from CDS):

Using observations from the Herschel Inventory of The Agents of Galaxy Evolution (HERITAGE) survey of the Magellanic Clouds (MC), we have found 35 evolved stars and stellar end products that are bright in the far-infrared. These 28 (LMC) and 7 (SMC) sources were selected from the 529 evolved star candidates in the HERITAGE far-infrared point source catalogs. Our source identification method is based on spectral confirmation, spectral energy distribution characteristics, careful examination of the multiwavelength images and includes constraints on the luminosity, resulting in a thoroughly vetted list of evolved stars. These sources span a wide range in luminosity and hence initial mass. We found 13 low- to intermediate-mass evolved stars, including asymptotic giant branch (AGB) stars, post-AGB stars, planetary nebulae, and a symbiotic star. We also identify 10 high mass stars, including 4 of the 15 known B[e] stars in the MC, 3 extreme red supergiants that are highly enshrouded by dust, a Luminous Blue Variable, a Wolf-Rayet star, and two supernova remnants. Further, we report the detection of 9 probable evolved objects which were previously undescribed in the literature. These sources are likely to be among the dustiest evolved objects in the MC. The Herschel emission may either be due to dust produced by the evolved star or it may arise from swept-up interstellar medium material.

Abstract Copyright: ∼

Journal keyword(s): circumstellar matter - infrared: stars - Magellanic Clouds - stars: late-type - stars: mass-loss - submillimeter: stars

VizieR on-line data: <Available at CDS (J/ApJ/811/145): table3.dat>

Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.

Simbad objects: 30

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Number of rows : 30
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 LHA 115-N 26 PN 00 48 08.624 -73 14 54.62 14.70 15.22 14.31   14.57 ~ 61 1
2 LHA 115-N 29 PN 00 48 36.526 -72 58 00.91 17.72 16.60 16.12 16.5 16.44 ~ 50 0
3 Jacoby SMC 17 PN 00 51 36.63 -73 20 17.0   18.347 18.036   17.242 Be 17 0
4 BMB-B 75 Mi* 00 52 12.9379490802 -73 08 53.136153620   17.05 15.31   12.86 M6.0 30 0
5 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
6 LHA 115-S 19 Sy* 00 54 19.5509270232 -72 29 11.522988024   18.57 18.27   17.70 ~ 21 0
7 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 7988 0
8 Brey 3a WR* 04 53 30.0791072664 -69 17 49.385662368 13.000 14.398 14.267 14.79 12.791 WC9 40 0
9 WOH G 64 Mi* 04 55 10.5236094912 -68 20 30.019011036       15.69 12.795 M7.5(I)e 110 0
10 HD 268835 s*b 04 56 47.0795205816 -69 50 24.769621212 10.21 10.77 10.63 10.72 10.16 B8[e] 119 0
11 [RP2006] J045855-685036 PN 04 58 55.29 -68 50 36.1 18.258 18.537 18.726   18.425 ~ 6 0
12 HD 269006 s*b 05 02 07.3942092168 -71 20 13.116800076 9.93 10.60 10.55 10.43 10.38 LBV 261 0
13 SSTISAGEMC J050451.97-683909.7 pA? 05 04 51.9929947440 -68 39 09.696052080 15.517 16.420 15.531 15.11 16.976 ~ 53 0
14 SMP LMC 28 pA? 05 07 57.620 -68 51 47.43 17.644 18.678 17.355 16.830 18.791 ~ 31 0
15 LHA 120-N 102 PN 05 08 03.3523991256 -68 40 16.560238548 15.580 16.298 15.406 14.86 16.653 ~ 51 0
16 Dachs LMC 1-11 HXB 05 13 42.6188050936 -67 24 10.097870616 12.969 13.750 13.632   13.113 B1: 23 0
17 OGLE LMC-LPV-31082 LP* 05 14 26.1359558064 -68 36 08.456108292         13.218 ~ 9 0
18 LHA 120-N 30 HII 05 14 34.4 -67 34 03           ~ 17 0
19 IRAS 05170-7156 LP* 05 16 18.720 -71 53 59.24           ~ 11 0
20 IRAS 05185-6806 Y*O 05 18 28.1480883000 -68 04 04.016015256           ~ 14 0
21 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
22 MCSNR J0525-6938 SNR 05 25 02.3 -69 38 39           ~ 446 1
23 OH 279.6-32.6 OH* 05 27 40.78 -69 08 05.7           ~ 26 1
24 SV* HV 2605 Em* 05 30 41.7389650464 -69 11 34.712550492 12.16 12.87 12.829 12.84 12.490 B1.5IIe 20 0
25 IRAS 05315-7145 AB* 05 30 44.10 -71 43 00.5           ~ 14 0
26 IRAS 05346-6949 LP* 05 34 14.4812357664 -69 47 20.557602348           ~ 22 0
27 SN 1987A SN* 05 35 27.98840 -69 16 11.1134           SNIIpec 5203 2
28 HD 37974 s*b 05 36 25.8534763728 -69 22 55.789571064 10.056 11.12 10.99 11.00 10.423 B0.5e 132 0
29 SV* HV 5999 s*r 05 41 21.6846102408 -69 31 48.818952732   15.16 13.06 11.80   M2.5Ia 18 0
30 IRAS 05495-7034 AB* 05 49 00.0419348088 -70 33 21.750361488           ~ 15 0

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