NEW VARIABLE STARS IN THE FIELD OF 66 OPH ON DIGITIZED MOSCOW PLATES

NEW VARIABLE STARS IN THE FIELD OF 66 OPH ON DIGITIZED MOSCOW PLATES

Regular photographic observations at the Moscow Observatory began in 1895. The archive of direct and spectroscopic sky photographs kept at the Sternberg Astronomical Institute (SAI) currently contains more than 60000 photographs. The most important part of the Moscow plate stacks are about 22500 dir...

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Main Authors: N. N. Samus, S. V. Antipin, D. M. Kolesnikova, L. A. Sat, K. V. Sokolovsky
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2010-12-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/85242
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spelling doaj-fbd70984e3ce4892bab3ff26203ee7382020-11-25T02:48:10ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152010-12-0123010.18524/1810-4215.2010.23.8524285242NEW VARIABLE STARS IN THE FIELD OF 66 OPH ON DIGITIZED MOSCOW PLATESN. N. Samus0S. V. AntipinD. M. KolesnikovaL. A. SatK. V. SokolovskyInstitute of Astronomy, Russian Academy of Sciences, 48 Pyatnitskaya Str., Moscow 119017, Russia; Sternberg Astronomical Institute, Moscow University, 13 University Ave., Moscow 119992, RussiaRegular photographic observations at the Moscow Observatory began in 1895. The archive of direct and spectroscopic sky photographs kept at the Sternberg Astronomical Institute (SAI) currently contains more than 60000 photographs. The most important part of the Moscow plate stacks are about 22500 direct sky photographs acquired in 1948–1996 with a 40-cm astrograph, at different sites in Crimea and near Moscow (currently in Nauchny, Crimea). The size of its plates is 30 x 30 cm, corresponding to a 10° x 10° sky field. The limiting magnitude is 17.5m for good-quality plates.http://oap.onu.edu.ua/article/view/85242
collection DOAJ
language English
format Article
sources DOAJ
author N. N. Samus
S. V. Antipin
D. M. Kolesnikova
L. A. Sat
K. V. Sokolovsky
spellingShingle N. N. Samus
S. V. Antipin
D. M. Kolesnikova
L. A. Sat
K. V. Sokolovsky
NEW VARIABLE STARS IN THE FIELD OF 66 OPH ON DIGITIZED MOSCOW PLATES
Odessa Astronomical Publications
author_facet N. N. Samus
S. V. Antipin
D. M. Kolesnikova
L. A. Sat
K. V. Sokolovsky
author_sort N. N. Samus
title NEW VARIABLE STARS IN THE FIELD OF 66 OPH ON DIGITIZED MOSCOW PLATES
title_short NEW VARIABLE STARS IN THE FIELD OF 66 OPH ON DIGITIZED MOSCOW PLATES
title_full NEW VARIABLE STARS IN THE FIELD OF 66 OPH ON DIGITIZED MOSCOW PLATES
title_fullStr NEW VARIABLE STARS IN THE FIELD OF 66 OPH ON DIGITIZED MOSCOW PLATES
title_full_unstemmed NEW VARIABLE STARS IN THE FIELD OF 66 OPH ON DIGITIZED MOSCOW PLATES
title_sort new variable stars in the field of 66 oph on digitized moscow plates
publisher Odessa I. I. Mechnykov National University
series Odessa Astronomical Publications
issn 1810-4215
publishDate 2010-12-01
description Regular photographic observations at the Moscow Observatory began in 1895. The archive of direct and spectroscopic sky photographs kept at the Sternberg Astronomical Institute (SAI) currently contains more than 60000 photographs. The most important part of the Moscow plate stacks are about 22500 direct sky photographs acquired in 1948–1996 with a 40-cm astrograph, at different sites in Crimea and near Moscow (currently in Nauchny, Crimea). The size of its plates is 30 x 30 cm, corresponding to a 10° x 10° sky field. The limiting magnitude is 17.5m for good-quality plates.
url http://oap.onu.edu.ua/article/view/85242
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AT dmkolesnikova newvariablestarsinthefieldof66ophondigitizedmoscowplates
AT lasat newvariablestarsinthefieldof66ophondigitizedmoscowplates
AT kvsokolovsky newvariablestarsinthefieldof66ophondigitizedmoscowplates
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