1998A&A...332...25G


Query : 1998A&A...332...25G

1998A&A...332...25G - Astronomy and Astrophysics, volume 33225-32 (1998/4-1)

Near-infrared photometry and optical spectroscopy of IRAS sources in the Small Magellanic Cloud.

GROENEWEGEN M.A.T. and BLOMMAERT J.A.D.L.

Abstract (from CDS):

Near-infrared photometry is obtained of 30 IRAS sources in the direction of the Small Magellanic Cloud selected to be possible AGB stars. Low resolution 4000 to 10000Å spectroscopy is presented for 10 of them, plus two AGB stars in the LMC. Improved IRAS fluxes are obtained using the gipsy package. Based on the optical spectra and analyses of colour-colour diagrams 9 are confirmed or likely carbon stars, and 8 are confirmed or likely oxygen-rich AGB stars. In three cases no near-infrared counterpart could be identified. The remaining 10 objects have the colours of mass-losing AGB stars, but not enough information is available to comment on the chemical type. In two of these cases there is a mismatch between the near-infrared and IRAS colours possibly indicating unusually large variability, or misidentification of the IRAS sources.

Abstract Copyright: ∼

Journal keyword(s): circumstellar matter - stars: mass loss - stars: AGB - Magellanic Clouds - infrared: stars

Nomenclature: Table 2: [GB98] SNNa (Nos 1-19, 20a-20b, 21-31)

CDS comments: Table 1 : [GB98] S8 is IRAS F00468-7427, not -7341.

Simbad objects: 49

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Number of rows : 49
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 HD 1274 PM* 00 16 36.8572514064 -63 51 37.396566468   10.83 10.00 9.5 9.435 G5V 20 0
2 V* BW Psc LP* 00 17 51.2408715576 +20 13 37.189434036   8.51 6.93     M3.5IIIa 30 0
3 * zet Tuc PM* 00 20 04.2586334956 -64 52 29.257190108 4.82 4.80 4.23 3.73 3.40 F9.5V 415 0
4 IRAS F00271-7120 C* 00 29 19.167 -71 03 49.97           C 5 0
5 IRAS 00350-7436 C* 00 36 59.5591952376 -74 19 50.255251536 16.88 15.81 14.47 14.25 12.92 C3,2e 32 0
6 IRAS F00356-7308 * 00 37 38.3 -72 52 14           ~ 3 0
7 IRAS F00388-7401 C* 00 40 43.855 -73 45 24.44         19.916 C 8 0
8 IRAS F00393-7326 C* 00 41 14.4169991976 -73 10 09.223734396     21.593   17.842 C 15 0
9 IRAS F00448-7332 C* 00 46 40.4260180584 -73 16 47.212061160     20.137   18.114 C 17 0
10 [GB98] S05 * 00 46 47.8 -73 27 55           ~ 2 1
11 RX J0047.2-7239 X 00 47 18.1 -72 39 48           ~ 19 2
12 IRAS F00454-7257 C* 00 47 18.9378112848 -72 40 34.073980788         19.242 C 13 1
13 IRAS F00468-7427 C* 00 48 35.688 -74 10 39.13           C 8 0
14 DEM S 58 As* 00 50 01 -72 26.2           ~ 10 0
15 IRAS 00483-7347 Mi* 00 50 07.1846249520 -73 31 25.137644700     22.532   16.016 M 39 0
16 IRAS F00486-7308 Mi* 00 50 30.6345902688 -72 51 29.885333040     17.089   13.391 M8II 29 0
17 IRAS F00490-7405 * 00 50 47.9 -73 49 12           ~ 3 0
18 IRAS 00491-7246 mul 00 50 54.9 -72 30 24           ~ 5 0
19 IRAS F00492-7408 * 00 50 57.3 -73 51 52           ~ 3 0
20 RAW 644 C* 00 50 57.3557867664 -72 30 12.132101808   21.04 17.73   14.75 C 11 0
21 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
22 IRAS F00530-7421 C* 00 54 42.685 -74 04 50.53     20.606   17.456 C 8 0
23 LHA 115-N 55 Em* 00 55 17.5530956784 -72 03 10.821105036 15.85 16.14 15.61   14.82 M:e 14 1
24 IRAS 00554-7351 C* 00 57 03.9450778464 -73 35 14.780611572         20.239 C 29 0
25 IRAS F00557-7309 C* 00 57 27.70 -72 53 28.0 20.61 21.18 20.87   18.72 C 15 0
26 SV* HV 11417 s*r 01 00 48.1661285976 -72 51 02.009778768 19.56 20.93 19.83   13.70 M5Ie 43 0
27 Cl* NGC 371 LE 29 s*r 01 03 02.4566119008 -72 01 53.002733736 17.09 16.98 14.03 13.48 11.693 K4.5-M4.5Ia-Iab 46 1
28 IRAS F01015-7222 * 01 03 08.1 -72 06 18           ~ 3 0
29 HD 6536 * 01 04 20.9804755008 -72 15 09.669137112 10.22 9.42 8.42     G8III 29 0
30 IRAS 01042-7215 LP* 01 05 49.314 -71 59 48.66 19.98 19.98 19.20   18.13 ~ 21 0
31 RAW 1543 C* 01 08 08.5513875600 -73 16 18.141917052   18.66 16.49   14.18 C 10 0
32 IRAS F01066-7332 AB* 01 08 10.3087049256 -73 15 52.510086828     20.393   14.788 M 18 0
33 NGC 419 OpC 01 08 17.26 -72 53 01.8 11.41 11.16 10.50   9.34 ~ 287 0
34 IRAS F01067-7308 * 01 08 17.8 -72 52 56           ~ 3 0
35 SV* HV 12956 Mi* 01 09 02.2609345848 -71 24 10.276925688 17.29 17.78 15.65   13.37 M5e 31 0
36 SV* HV 2084 s*r 01 09 38.2081762584 -73 20 02.225692176   13.690 11.797     M2Ia 42 0
37 IRAS F01091-7320 C* 01 10 32.244 -73 05 04.07           C 10 0
38 HD 7644 * 01 15 37.3805399592 -45 26 36.254766156   10.89 10.29     F6V 10 0
39 V* Z Psc C* 01 16 05.0304050160 +25 46 09.689905056 12.85 9.46 6.84     C-N5 184 0
40 IRAS F01160-7451 LP* 01 17 17.3043054288 -74 36 16.993321992           ~ 6 0
41 IRAS F01210-7125 C* 01 22 28.2875562888 -71 09 26.022141432           C 8 0
42 IRAS F01238-7218 * 01 25 10.3 -72 03 16           K1/K2III 2 0
43 CPD-69 177 WD* 03 10 31.0195960176 -68 36 03.380768388 10.757 11.413 11.394 11.47 11.558 DA3.0 299 0
44 IRAS 04496-6958 C* 04 49 18.4933717920 -69 53 14.430196680 20.060 20.027 18.791   15.060 C 50 0
45 MSX LMC 310 C* 05 20 19.3893585384 -66 35 47.797132596         14.825 C 24 0
46 [KDM2001] 3409 C* 05 20 21.6159799056 -66 36 04.199381388   16.21   14.72   C 20 0
47 CD-44 12736 PM* 18 36 25.9502475648 -44 18 36.907592904   10.83 10.22     G0 222 0
48 * 19 Psc C* 23 46 23.5164473376 +03 29 12.519049272 10.95 7.62 5.02 3.19 1.82 C-N6 462 0
49 IRAS F00448-7344 IR ~ ~           ~ 2 0

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