Peremennye Zvezdy

Article in PDF
"Peremennye Zvezdy",
Prilozhenie
,
vol. 9, N 35 (2009)

Mira Variables from the MACHO Galactic Bulge Scutum Fields

J. Greaves
Northants, England, UK

ISSN 2221–0474

Received:   16.12.2009;   accepted:   23.12.2009
(E-mail for contact: knot@safe-mail.net)


#NameOtherCoord (J2000)TypeMaxMinSystemPeriodEpoch (JD)typeSpCommentL.CurveFind.ChartData
1 MACHO 301.45271.1818 31 27.0, -13 39 44M14.617.6R241.72450644max  301_45271_18.gif 301_45271_18.txt
2 MACHO 301.45446.2418 31 29.1, -13 11 15M14.818.2R213.22451348max  301_45446_24.gif 301_45446_24.txt
3 MACHO 301.45607.2318 31 52.2, -13 39 05M13.116.3R216.82451360max  301_45607_23.gif 301_45607_23.txt
4 MACHO 301.45778.7218 32 12.0, -13 27 31M15.217.8R242.62451293max  301_45778_72.gif 301_45778_72.txt
5 MACHO 301.45950.2618 32 23.4, -13 13 08M14.117.7R298.82451280max  301_45950_26.gif 301_45950_26.txt
6 MACHO 301.46117.1918 32 44.6, -13 18 40M15.218.5R237.02450603max  301_46117_19.gif 301_46117_19.txt
7 MACHO 301.46286.1018 33 07.3, -13 13 40M15.018.9R285.02450468max  301_46286_10.gif 301_46286_10.txt

Remarks:
Presented are the details for seven Mira variables found from the Scutum MACHO Galactic Bulge field 301 epoch photometry as publicly served via their new Virtual Observatory interface (Smillie 2009) and as downloaded and sourced via TOPCAT.

Each object was checked against the Strasbourg CDS Vizier service for pre-existence as a Mira in variability catalogues.

The astrometric positions were derived from the Carlsberg Meridian Catalog 14 (CMC14 2006).

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. The application TOPCAT (http://www.starlink.ac.uk/topcat) was used for VO access and visualisation of the data. Catalogue data served by the VizieR service of the CDS, Strasbourg, was used in this analysis.

References:
CMC14, 2006, Carlsberg Meridian Catalog 14, Centre de Donnees Astronomiques de Strasbourg, I/304
Smillie, J. G., for the MACHO collaboration, 2009, arXiv:0910.5041



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