2020MNRAS.498.2263R


Query : 2020MNRAS.498.2263R

2020MNRAS.498.2263R - Mon. Not. R. Astron. Soc., 498, 2263-2269 (2020/October-3)

Further milliarcsecond resolution results on cool giants and binary stars from lunar occultations at Devashtal.

RICHICHI A., SHARMA S., SINHA T., PANDEY R., GHOSH A., OJHA D.K., PANDEY A.K. and NAIK M.B.

Abstract (from CDS):

We report on 26 lunar occultation events observed in the context of a programme started at Devasthal in 2017. In addition to the customary observations with the 1.3-m telescope, we report here also the first attempts performed with the TIRCAM2 camera at the 3.6-m Devasthal Optical Telescope in the near-infrared (near-IR). The results consist in the first-time angular diameters for two late-type giants, in a measurement of the well-known asymptotic giant branch pulsating variable SW Vir, and in the measurement of eight small separation binaries one of which is detected for the first time (HR 1860). We also measured the wider binaries SAO 94431 and 55 Tau (twice). The remaining sources were found to be unresolved with upper limits as small as 1 mas. We plan to develop further the high-speed capability of the TIRCAM2 instrument, so as to include in our programme also more near-IR, highly extincted sources.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): occultations - stars: atmospheres - binaries: general

Simbad objects: 25

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Number of rows : 25
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 V* FG Psc LP* 00 21 08.8971967200 -02 21 24.943292064   10.99 9.72     M5 6 0
2 * 85 Cet ** 02 42 28.9370887128 +10 44 30.224220144   6.36 6.31     A2V 50 0
3 * mu. Cet SB* 02 44 56.5373458591 +10 06 50.921738061   4.57 4.26     A9IIIp 201 0
4 BD+13 576 PM* 03 38 31.9571603400 +13 36 21.477215988   9.49 8.94     F8 24 0
5 HD 22682 PM* 03 39 17.0529763848 +13 53 29.381962596 8.180 7.570 6.670     G5 44 0
6 HD 26380 * 04 10 55.1692650024 +15 56 47.934139524   7.32 7.17     A0 27 0
7 HD 27029 * 04 16 48.6891598080 +16 12 51.791381964 8.670 7.670 6.560     G8III 21 0
8 * 55 Tau ** 04 19 54.8606314218 +16 31 21.225588133   7.401 6.853     F8V 257 0
9 * alf Tau LP? 04 35 55.23907 +16 30 33.4885 4.32 2.40 0.86 -0.37 -1.31 K5+III 1298 2
10 HD 29496 C*? 04 39 20.2648036104 +16 45 14.814251028   10.44 8.42     N? 9 0
11 HD 34251 ** 05 16 43.88190 +18 26 22.3320           B3V+B6V 30 0
12 IRAS 05255+1832 LP* 05 28 29.0795314128 +18 34 28.156906416   12.15 10.25 9.46   M3.0III 7 0
13 HD 36230 * 05 31 05.0453592720 +20 11 20.937893892   10.00 8.17     K5 7 0
14 HD 36589 V* 05 33 38.8369609800 +20 28 27.190778340   6.151 6.189     B6V 55 0
15 HD 46467 PM* 06 34 27.5900253888 +21 25 37.872692832   9.09 7.97     K2 19 0
16 V* AX Gem AB* 06 37 06.7577146680 +21 07 03.496585188   10.72 9.45     M5 20 0
17 HD 261221 SB* 06 39 14.7057888408 +21 16 44.257600272   9.67 8.63     K0 8 0
18 V* RU Pup C* 08 07 29.8292965296 -22 54 45.272487204   12.07 8.45 7.35   C-N5III: 71 0
19 HD 81540 * 09 26 37.8822695424 +16 41 53.884686840 11.400 9.580 7.970     M2.5III 27 0
20 * psi Leo V* 09 43 43.9068253008 +14 01 18.131099484 8.93 6.98 5.35     M2III 74 0
21 BD+14 2146 ** 09 47 36.7491 +14 18 46.881   9.94 9.39     F8 9 0
22 V* SW Vir AB* 13 14 04.3830437280 -02 48 25.130666916 9.24 8.52 6.85     M7III: 274 0
23 HD 147474 * 16 22 51.9106685112 -17 09 10.581009264   10.15 8.92     K0III 11 0
24 * 21 Sgr * 18 25 21.0394302144 -20 32 30.022206936   6.32 4.86     K1/2III 65 0
25 HD 221925 ** 23 36 17.49209 -07 07 01.9903   8.16 7.84     F0V 20 0

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