2006A&A...452..571P


Query : 2006A&A...452..571P

2006A&A...452..571P - Astronomy and Astrophysics, volume 452, 571-577 (2006/6-3)

Spectroscopic observations of the rapid rotating post-AGB star IRAS 05381+1012.

PEREIRA C.B. and ROIG F.

Abstract (from CDS):

We report on the high-resolution stellar parameters and abundance analysis of the rapidly rotating post-AGB star IRAS 05381+1012. Analysis of high-resolution spectra shows that IRAS 05381+1012 has an effective temperature of Teff=5200± 100K and a surface gravity of logg=1.0±0.5 corresponding to a spectral type G(2-3)I. These parameters result in an estimated luminosity of 970L and a distance of 2700pc. We also show that IRAS 05381+1012 has a projected rotational velocity vsini=40±10km/s. The abundance analysis based on a few available lines reveals that this star is an iron-deficient object with [Fe/H]=-0.8. We also analyze the abundance pattern and compare it to other classes of stars with similar stellar parameters.

Abstract Copyright:

Journal keyword(s): stars: AGB and post-AGB - stars: abundances

CDS comments: In ref list HAMUY et al. 1994 is 1994PASP..106..566H instead of 1994AJ....108.2226H.

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 - 2023
#notes
1 HD 9973 Em* 01 39 07.1682962592 +61 04 44.735125980 8.51 7.741 6.911     F5Iab 78 0
2 HD 246299 pA* 05 40 57.0542926512 +10 14 24.972372852   11.36 10.54 10.25   G2I 26 0
3 HD 289002 * 06 45 13.3725491952 +02 08 14.685250596 10.06 10.62 10.44     B1 251 0
4 V* V421 CMa pA* 07 16 08.2750036896 -23 27 01.536458868   11.16 10.73     F5 29 0
5 EM* AS 201 PN 08 31 42.8828281680 -27 45 31.543524864   13 11.80     F9III 88 0
6 CD-32 5613 WD* 08 41 32.4290850497 -32 56 32.915823461   12.07 11.85 12.3   DA5.5 291 0
7 HD 89353 pA* 10 18 07.5899342712 -28 59 31.195183524   5.76 5.53     B9.5Ib/II 302 0
8 V* V Hya C* 10 51 37.2615873024 -21 15 00.333928044   12.23 6.80 7.42   C-N:6 357 0
9 V* V802 Car pA* 11 02 04.3154924592 -62 09 42.834006396   9.57 8.90 9.38   F2III 51 0
10 CD-53 4543 pA* 12 20 15.0622728552 -53 55 31.444773420 10.29 9.74 9.36 9.69   A7I 42 0
11 HD 107369 pA* 12 20 44.9452565208 -32 33 26.107102908   9.78 9.60     A2II/III 38 0
12 HD 108015 pA* 12 24 53.5035641784 -47 09 07.499485656   8.379 7.96     F3/5Ib/II 58 0
13 WG 22 WD* 12 38 49.7811220835 -49 48 00.219515411   14.14 13.96     DA4.2 221 0
14 V* LN Hya pA* 12 56 30.1302499344 -26 27 37.047715704   9.104 8.697   9.291 F3Ia 114 0
15 V* EN TrA pA* 14 57 00.6850828200 -68 50 22.897081716   9.42 8.70     F2Ib 72 0
16 HD 133656 pA* 15 07 27.4396006536 -48 17 53.894056668 8.09 7.88 7.58 8.45   A5Iab 49 0
17 Cl* NGC 5904 MSB 1 AB* 15 18 34.117 +02 05 00.17   14.2150 12.2791   14.6608 ~ 30 4
18 HD 330036 PN 15 51 15.9290064932 -48 44 58.559111355   11.759 10.892 10.921   F5III-IVe 155 0
19 HD 148743 pA* 16 30 30.0183563616 -07 30 52.031445516 6.94 6.824 6.461     A7Ib 92 0
20 CD-53 7049 PN 17 03 02.8784604504 -53 55 53.966024508   11.84 11.48     B/Ae 63 1
21 HD 161796 pA* 17 44 55.4694563472 +50 02 39.482823336 8.00 7.68 7.21 6.77 6.51 F3Ib 320 0
22 * 89 Her pA* 17 55 25.1883476136 +26 02 59.968457664 5.36 5.70 5.36 5.06 4.94 F2Ibp 403 0
23 HD 341617 pA* 18 08 20.0857525920 +24 10 43.321447236   11.41 11.39     B1IIIe 84 0
24 HD 172481 pA* 18 41 36.9595215744 -27 57 01.235714652   9.58 9.06     F2/3Ia 48 0
25 IRAS 19386+0155 pA* 19 41 08.2923311712 +02 02 31.208770140   12.32 11.20     F5Ib 38 0
26 BD-13 5550 pA* 20 01 49.8291561312 -12 41 17.767855176 10.62 11.3 11.4     B1Ibe 73 0
27 V* V1401 Aql pA* 20 05 05.4136151160 -11 35 57.894584100   6.88 6.39     F2II 100 0
28 M 15 GlC 21 29 58.33 +12 10 01.2           ~ 3073 0
29 PN Ps 1 PN 21 29 59.38 +12 10 27.5   13.39 14.06     sdO 282 0
30 EM* StHA 190 Sy* 21 41 44.8876442736 +02 43 54.414342804   11.13 10.22     G5e 47 0

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2023.03.27-06:28:40

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