Автор | D Kunneriath |
Автор | A Eckart |
Автор | S Vogel |
Автор | L Sjouwerman |
Автор | H Wiesemeyer |
Автор | R Schödel |
Автор | F K Baganoff |
Автор | M Morris |
Автор | T Bertram |
Автор | M Dovciak |
Автор | D Dowries |
Автор | W J Duschl |
Автор | V Karas |
Автор | S Konig |
Автор | T Krichbaum |
Автор | M Krips |
Автор | R-S Lu |
Автор | S Markoff |
Автор | J Mauerhan |
Автор | L Meyer |
Автор | J Moultaka |
Автор | K Muzic |
Автор | F Najarro |
Автор | K Schuster |
Автор | C Straubmeier |
Автор | C Thum |
Автор | G Witzel |
Автор | M Zamaninasab |
Автор | A Zensus |
Дата выпуска | 2008-10-01 |
dc.description | At the center of the Milky Way, with a distance of ∼8 kpc, the compact source Sagittarius A* (SgrA*) can be associated with a super massive black hole of ∼4x 10<sup>6</sup>M<sub>⊙</sub>. SgrA* shows strong variability from the radio to the X-ray wavelength domains. Here we report on simultaneous NIR/sub-millimeter/X-ray observations from May 2007 that involved the NACO adaptive optics (AO) instrument at the European Southern Observatory's Very Large Telescope, the Australian Telescope Compact Array (ATCA), the US mm-array CARMA, the IRAM 30m mm-telescope, and other telescopes. We concentrate on the time series of mm/sub-mm data from CARMA, ATCA, and the MAMBO bolometer at the IRAM 30m telescope. |
Формат | application.pdf |
Издатель | Institute of Physics Publishing |
Копирайт | © 2008 IOP Publishing Ltd |
Название | Coordinated mm/sub-mm observations of Sagittarius A* in May 2007 |
Тип | paper |
DOI | 10.1088/1742-6596/131/1/012006 |
Electronic ISSN | 1742-6596 |
Print ISSN | 1742-6588 |
Журнал | Journal of Physics: Conference Series |
Том | 131 |
Первая страница | 12006 |
Последняя страница | 12012 |
Выпуск | 1 |