Набор мебели для спальни “Нинель”. Изделие изготовлено из плиты древесностружечной, крышки – из плиты МДФ облицованы шпоном строганным с лицевой стороны. Декоративные бруски на дверях шкафа, стенках передних ящиков и спинках кровати, карниз и цоколь шкафа, вертикальные опорные бруски кровати из массива древесины дуба. Двери в закрытом положении фиксируются петлёй и открываются с помощью ручки-кнопки. Отделка «севрес» с патиной. Габаритные размеры: Комод MM-167-04 - B796 х H876 х T445 mm Зеркало MM-167-05 - H660 х B1010 х T29 mm Шкаф для одежды 4-x дверный MM-167-01/04 - B2010 х H2237 х T617 mm Кровать MM-167-02/16Б - B1688 х H1000 х T2106 mm Тумба прикроватная MM-167-03 - B500 х H442 х T441 mm Шкаф для одежды 3-х дверный «Нинель» (1/02) MM-167-01/03 - B1528 х H2237 х T617 mm
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Набор мебели для спальни “Нинель”. Изделие изготовлено из плиты древесностружечной, крышки – из плиты МДФ облицованы шпоном строганным с лицевой стороны. Декоративные бруски на дверях шкафа, стенках передних ящиков и спинках кровати, карниз и цоколь шкафа, вертикальные опорные бруски кровати из массива древесины дуба. Двери в закрытом положении фиксируются петлёй и открываются с помощью ручки-кнопки. Отделка «севрес» с патиной. Габаритные размеры: Комод MM-167-04 - B796 х H876 х T445 mm Зеркало MM-167-05 - H660 х B1010 х T29 mm Шкаф для одежды 4-x дверный MM-167-01/04 - B2010 х H2237 х T617 mm Кровать MM-167-02/16Б - B1688 х H1000 х T2106 mm Тумба прикроватная MM-167-03 - B500 х H442 х T441 mm Шкаф для одежды 3-х дверный «Нинель» (1/02) MM-167-01/03 - B1528 х H2237 х T617 mm
Jamesrak
Здравствуйте! Я Алексей. В приложении 2ГИС заметил рейтинг Вашей фирмы. Мы занимаемся написанием отзывов. На один отрицательный отзыв мы пишем 10 положительных отзывов для Вашей организации в 2ГИС. Это не очень дорого и дает возможность получить дополнительных клиентов, которые выбирают среди фирм по Вашему направлению в мобильном приложении 2GIS по отзывам. Скажите, мог бы я направить Вам наше предложение? Адрес для обратной связи: 2gis@re-put.ru С уважением, Алексей RE-PUT.ru 2GIS/Yandex/Google карты
Michaelhause
Possibilities The authors of the study, published May 6 in the journal Monthly Notices of the Royal Astronomical Society, specifically set out to search for Dyson spheres, in the form of infrared heat near stars that couldn’t be explained in any other way. <a href=https://kra31att.cc>kraken сайт</a> Using historical data from telescopes that pick up infrared signatures, the research team looked at stars located within less than 1,000 light-years from Earth: “We started with a sample of 5 million stars, and we applied filters to try to get rid of as much data contamination as possible,” said lead study author Matias Suazo, a doctoral student in the department of physics and astronomy of Uppsala University in Sweden. “So far, we have seven sources that we know are glowing in the infrared but we don’t know why, so they stand out.” https://kra31att.cc kraken onion There is no conclusive evidence that the seven stars have Dyson spheres around them, Suazo cautioned. “It’s difficult for us to find an explanation for these sources, because we don’t have enough data to prove what is the real cause of the infrared glow,” he said. “They could be Dyson spheres, because they behave like our models predict, but they could be something else as well.” Among the natural causes that could explain the infrared glow are an unlucky alignment in the observation, with a galaxy in the background overlapping with the star, planetary collisions creating debris, or the fact that the stars may be young and therefore still surrounded by disks of hot debris from which planets would later form. The data used by the researchers comes from two active space telescopes — the Wide-field Infrared Survey Explorer, or WISE, from NASA and Gaia from the European Space Agency — as well as an astronomical survey of the sky in infrared light called The Two Micron All Sky Survey. Also known as 2MASS, the collaboration between the University of Massachusetts and the US space agency’s Jet Propulsion Laboratory took place between 1997 and 2001.
Mayoxy
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ThomasSoora
Dokumenty kolekcjonerskie to niezwykle ciekawy obszar dla milosników historii i kultury materialnej. Obejmuje szeroki zakres artefaktów, takich jak stare paszporty, dowody osobiste, prawa jazdy, bilety czy legitymacje. Kolekcjonowanie takich dokumentów moze byc pasjonujacym hobby, pozwalajacym na zglebianie historii i obyczajów róznych epok. Jednakze, ze wzgledu na swój charakter, dokumenty te budza równiez pewne kontrowersje, szczególnie w kontekscie ich ewentualnego wykorzystania w sposób niezgodny z prawem. Historia dokumentów kolekcjonerskich Kolekcjonowanie dokumentów ma swoje korzenie w XIX wieku, kiedy to zainteresowanie historia i archeologia zaczelo rosnac wsród zamozniejszych warstw spolecznych. Z czasem, obok starozytnych rekopisów i ksiazek, pojawilo sie równiez zainteresowanie dokumentami o bardziej wspólczesnym charakterze, takimi jak bilety z wydarzen kulturalnych, legitymacje czy inne przedmioty zwiazane z codziennym zyciem. W XX wieku, zwlaszcza po I wojnie swiatowej, dokumenty takie jak paszporty czy dowody osobiste zaczely byc postrzegane jako cenne pamiatki rodzinne, a takze interesujace obiekty dla kolekcjonerów. Ich wartosc wynikala nie tylko z ich rzadkosci, ale takze z kontekstu historycznego, w jakim powstaly i byly uzywane. Wartosc dokumentów kolekcjonerskich Wartosc dokumentów kolekcjonerskich zalezy od wielu czynników, takich jak ich stan, wiek, rzadkosc oraz historyczne znaczenie. Na przyklad, paszport z okresu miedzywojennego nalezacy do znanej postaci historycznej moze osiagnac na aukcjach wysoka cene. Z kolei bilety z waznych wydarzen sportowych czy koncertów moga byc poszukiwane przez kolekcjonerów z calego swiata. Wartosc dokumentów czesto wzrasta, gdy sa one zwiazane z waznymi momentami w historii, takimi jak wojny, rewolucje, czy zmiany polityczne. Na przyklad, dokumenty z czasów PRL-u, takie jak legitymacje partyjne czy przepustki graniczne, moga byc szczególnie cenione przez kolekcjonerów zainteresowanych historia Polski. czytaj dalej https://dobreplastiki.com/pl/
Mayoxy
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Jameslup
Possibilities The authors of the study, published May 6 in the journal Monthly Notices of the Royal Astronomical Society, specifically set out to search for Dyson spheres, in the form of infrared heat near stars that couldn’t be explained in any other way. <a href=https://kra31att.cc>kraken даркнет</a> Using historical data from telescopes that pick up infrared signatures, the research team looked at stars located within less than 1,000 light-years from Earth: “We started with a sample of 5 million stars, and we applied filters to try to get rid of as much data contamination as possible,” said lead study author Matias Suazo, a doctoral student in the department of physics and astronomy of Uppsala University in Sweden. “So far, we have seven sources that we know are glowing in the infrared but we don’t know why, so they stand out.” https://kra31att.cc kraken зайти There is no conclusive evidence that the seven stars have Dyson spheres around them, Suazo cautioned. “It’s difficult for us to find an explanation for these sources, because we don’t have enough data to prove what is the real cause of the infrared glow,” he said. “They could be Dyson spheres, because they behave like our models predict, but they could be something else as well.” Among the natural causes that could explain the infrared glow are an unlucky alignment in the observation, with a galaxy in the background overlapping with the star, planetary collisions creating debris, or the fact that the stars may be young and therefore still surrounded by disks of hot debris from which planets would later form. The data used by the researchers comes from two active space telescopes — the Wide-field Infrared Survey Explorer, or WISE, from NASA and Gaia from the European Space Agency — as well as an astronomical survey of the sky in infrared light called The Two Micron All Sky Survey. Also known as 2MASS, the collaboration between the University of Massachusetts and the US space agency’s Jet Propulsion Laboratory took place between 1997 and 2001.