1996A&A...312..521M


Query : 1996A&A...312..521M

1996A&A...312..521M - Astronomy and Astrophysics, volume 312521-524 (1996/8-2)

Optical and near-infrared photometry of the Vega-excess star SAO 26804=HD 233517.

MIROSHNICHENKO A.S., BERGNER Y.K. and KURATOV K.S.

Abstract (from CDS):

UBVRIJHK photometry of the Vega-excess star SAO 26804=HD 233517and several stars of its environments obtained at the 1-meter telescope of the Tien-Shan Observatory in Kazakhstan is presented. It is shown that the star has a later spectral type than has been considered previously. Its effective temperature is estimated by the visual surface brightness method as 4170K. The star has no excess radiation in the range of 0.3-2.5µm. A comparison of its IR-excesses with those of other K-type stars with IR-excesses is made. HD 233517 is probably more evolved than SAO 179815=HD 98800 having a very similar intrinsic spectral energy distribution (SED) and the largest IR-excess among K-type stars from the SAO catalogue.

Abstract Copyright: ∼

Journal keyword(s): circumstellar matter - stars: individual: HD 233517 - infrared: stars

Simbad objects: 9

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Number of rows : 9
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 * eps Eri BY* 03 32 55.8444911587 -09 27 29.739493865 5.19 4.61 3.73 3.00 2.54 K2V 2073 1
2 HD 69682 PM* 08 20 29.0945189208 +53 34 26.725574928 6.880 6.810 6.510     kA8hF0mF3IIIBa 50 0
3 HD 233517 RG* 08 22 46.7147840400 +53 04 49.230337440   10.85 9.71     K2 98 0
4 HD 233520 * 08 22 51.1396592040 +53 04 10.806153168   10.23 9.22     K0 5 0
5 HD 70313 PM* 08 23 48.5013137736 +53 13 10.965328104 5.760 5.660 5.540   5.38 A3Va 80 0
6 HD 70919 PM* 08 26 59.4729215304 +53 37 44.894134056 8.200 8.140 7.900     F0 15 0
7 * omi UMa PM* 08 30 15.8701566400 +60 43 05.405606188 4.79 4.27 3.42 2.76 2.31 G5III: 271 1
8 HD 98800 TT* 11 22 05.28975 -24 46 39.7571   10.20 9.28 9.26 7.386 K5V(e) 401 0
9 HD 221354 PM* 23 31 22.2087431778 +59 09 55.867801045   7.57   6.2   K0V 190 0

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