| Article in PDF |
"Peremennye Zvezdy", Prilozhenie, vol. 11, N 12 (2011) |
| ISSN 2221–0474 |
Received: 22.01.2011; accepted: 5.04.2011
(E-mail for contact: klaus.bernhard@liwest.at)
|
Comments:
1. J–K = 1.483 (2MASS), AKARI/IRC 1804195–272448.
2. J–K = 1.466 (2MASS), AKARI/IRC 1804300–271417.
3. J–K = 1.690 (2MASS), AKARI/IRC 1804439–272833.
4. J–K = 1.709 (2MASS), AKARI/IRC 1804472–272146.
5. J–K = 1.432 (2MASS).
6. J–K = 1.619 (2MASS), AKARI/IRC 1805096–270503.
7. J–K = 1.619 (2MASS), AKARI/IRC 1805158–271645.
8. J–K = 1.521 (2MASS), AKARI/IRC 1805227–270612.
9. J–K = 1.904 (2MASS), AKARI/IRC 1805205–270139.
10. J–K = 1.489 (2MASS).
11. J–K = 1.743 (2MASS), AKARI/IRC 1806044–272345.
12. J–K = 1.477 (2MASS).
13. J–K = 1.805 (2MASS), AKARI/IRC 1806021–270317.
14. J–K = 1.524 (2MASS).
15. J–K = 1.541 (2MASS), AKARI/IRC 1806085–272639.
16. J–K = 1.476 (2MASS).
17. J–K = 1.597 (2MASS), AKARI/IRC 1806315–271654.
18. J–K = 1.427 (2MASS).
19. J–K = 1.449 (2MASS), AKARI/IRC 1808482–275043.
20. J–K = 1.559 (2MASS), AKARI/IRC 1808484–274925.
21. J–K = 1.631 (2MASS), AKARI/IRC 1808481–272233.
22. J–K = 1.364 (2MASS).
23. Mis V0053. J–K = 1.287 (2MASS).
24. J–K = 1.624 (2MASS), AKARI/IRC 1809140–274023.
25. J–K = 2.079 (2MASS), AKARI/IRC 1809417–280504.
26. J–K = 1.697 (2MASS), AKARI/IRC 1809358–272947.
27. J–K = 1.511 (2MASS), AKARI/IRC 1810056–275632.
28. J–K = 1.823 (2MASS), AKARI/IRC 1810064–274647.
29. J–K = 2.216 (2MASS), AKARI/IRC 1810170–273030.
30. J–K = 1.668 (2MASS).
31. J–K = 1.67. (2MASS)
32. J–K = 1.762 (2MASS), AKARI/IRC 1810487–275623.
33. J–K = 1.33. (2MASS)
34. J–K = 1.396 (2MASS), AKARI/IRC 1812207–274356.
35. J–K = 1.394 (2MASS).
36. J–K = 1.748 (2MASS), AKARI/IRC 1812486–273852.
37. J–K = 1.793 (2MASS), AKARI/IRC 1812311–271117.
38. J–K = 1.737 (2MASS), AKARI/IRC 1813207–273830.
39. J–K = 1.571 (2MASS), AKARI/IRC 1803025–273438.
40. J–K = 1.855 (2MASS), AKARI/IRC 1803071–280538.
41. J–K = 1.574 (2MASS).
42. J–K = 1.477 (2MASS), AKARI/IRC 1803069–274208.
43. J–K = 1.592 (2MASS), AKARI/IRC 1803126–273528.
44. J–K = 2.371 (2MASS), AKARI/IRC 1803128–272807.
45. J–K = 1.737 (2MASS), AKARI/IRC 1803061–272600.
46. J–K = 2.152 (2MASS), AKARI/IRC 1803361–274404.
47. J–K = 1.539 (2MASS).
48. J–K = 1.985 (2MASS), AKARI/IRC 1803462–274308.
49. J–K = 1.690 (2MASS), AKARI/IRC 1804439–272833.
50. J–K = 1.762 (2MASS).
51. J–K = 1.529 (2MASS).
52. J–K = 1.738 (2MASS).
53. J–K = 1.535 (2MASS).
54. J–K = 1.344 (2MASS).
55. J–K = 1.544 (2MASS).
56. J–K = 1.418 (2MASS).
57. J–K = 1.637 (2MASS), AKARI/IRC 1806565–275834.
58. J–K = 2.338 (2MASS), AKARI/IRC 1806471–275243.
59. J–K = 1.549 (2MASS), AKARI/IRC 1807199–281501.
60. J–K = 1.674 (2MASS), AKARI/IRC 1807150–275416.
61. J–K = 1.613 (2MASS).
62. J–K = 1.577 (2MASS), AKARI/IRC 1807482–281301.
63. J–K = 1.630 (2MASS), AKARI/IRC 1807438–281302.
64. J–K = 1.519 (2MASS), AKARI/IRC 1807507–280915.
65. J–K = 1.468 (2MASS).
66. J–K = 1.743 (2MASS), AKARI/IRC 1807573–281448.
67. J–K = 2.145 (2MASS), AKARI/IRC 1808043–281055.
68. J–K = 1.440 (2MASS), AKARI/IRC 1808071–280353.
69. J–K = 1.584 (2MASS).
70. J–K = 1.518 (2MASS).Remarks:
Details are presented for seventy Mira variables found from the MACHO Galactic Bulge fields 101-105 epoch photometry (http://wwwmacho.anu.edu.au/ or http://macho.anu.edu.au/). The Macho R magnitudes were calculated from the given instrumental R magnitudes using the formula given in Alcock et al. (1999). The programme AVE (Analisis de Variabilidad Estelar, Grup d'Estudis Astronomics) was used for the data analysis.
Each object was checked against the Strasbourg CDS Vizier service and the International Variable Star Index for pre-existence as an Mira type star in variability catalogues.
The astrometric positions were derived from the 2MASS catalog (Skrutskie et al. 2006). In the Comments, we present near-infrared color indices from the 2MASS catalog and, whenever available, identifications with the "Mid-Infrared All-Sky Survey" (Ishihara et al. 2010).
Acknowledgements: This paper utilizes public domain data obtained by the MACHO Project, jointly funded by the US Department of Energy through the University of California, Lawrence Livermore National Laboratory under contract No. W-7405-Eng-48, by the National Science Foundation through the Center for Particle Astrophysics of the University of California under cooperative agreement AST-8809616, and by the Mount Stromlo and Siding Spring Observatory, part of the Australian National University. Catalogue data served by the VizieR service of the CDS, Strasbourg, was used in this analysis. It is a pleasure to thank John Greaves for helpful suggestions and comments.References:
Alcock, C., Allsman, R.A., Alves, D.R., et al., 1999, Publ. of Astron. Society of Pacific, 111, 1539
Ishihara, D., Onaka, T., Kataza, H., et al., 2010, Astron. Astrophys., 514, A1
Skrutskie, M.F., Cutri, R.M., Stiening, R., et al., 2006, AJ, 131, 1163
