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NOVA CARINAE 2018 - ASASSN-18fv |
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Load higher resolution without Nova labeling 1800 x 1200 Pixel Load higher resolution with Nova labeling 1800 x 1200 Pixel |
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Load higher resolution without Nova labeling 1800 x 1200 Pixel Load higher resolution with Nova labeling 1800 x 1200 Pixel |
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Load higher resolution without Nova labeling 1800 x 1200 Pixel Load higher resolution with Nova labeling 1800 x 1200 Pixel |
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Nova Carinaon May 2019 load large image with Nova labeling 1400 x 1200 Pixel |
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Object description - Nova Carinae 2018 - with the provisional
designation ASASSN-18fv The Nova Carinae was discovered on images taken on 20 March 2018 with a telescope of the project "All Sky Automated Survey for SuperNovae" (ASAS-SN). ASAS is a system of several automated, web-controlled telescopes distributed all over the world, so that the sky can be monitored from both the northern and southern hemispheres. The system is mainly used to search for novae, supernovae and other events where astronomical objects change their brightness within a short time. At the time of discovery, the brightness of the Nova was brighter than 10th magnitude. The star is positioned just west of the large Carina star formation area NGC 3372 and directly south of the star HD 92 063 of the 5th magnitude. The celestial coordinates of the Nova (epoch J 2000) are: Rectacension: 10h 36m 13.7s, Declination: -59° 35´55". We were very lucky that one of us (Paech) was in Namibia from March 21 to April 20. Despite the still prevailing rainy season, some good pictures of the Nova Carinae could be taken on two clear nights. |
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Spectroscopic observations of the star on March 21 show a strong
stellar continuum and narrow emission lines which could indicate that this
event is not a classical nova, but that it cannot be definitively excluded. The
star seems to belong to the Carina nebulaecomplex and so the event could also
be a strong eruption of a very young star. What exactly triggered the increase in brightness will only become apparent later on. Images of the position before the eruption of the GAIA satellite show a star of the 20th magnitude. On 21 March the brightness had already risen to the 6.5 magnitude. When we return to Onjala in July 2018, it will be exciting to see the Nova region again. Perhaps by then professional astronomers will have clarified whether it is a classic Nova or a far more exotic event. |
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At the end
of July we could take more pictures of the Nova Carinae. Interestingly, and
strangely enough, there are no scientific publications on this event that
clarify what kind of novatype it is. In any case, the brightness of the nova in
July (4 months after its discovery) was still so high that the star could be
easily observed photographically. |
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All Images and all Content are © by Franz Hofmann + Wolfgang Paech |