IC 2497 and Hanny's Voorwerp. Technical card Imaging telescopes or lenses:Home made 400mm F/4 Newtonian. Imaging cameras:Quantum Scientific Imaging QSI583wsg. Mounts:10 Micron GM2000 QCI. Guiding telescopes or lenses:Home made 400mm F/4 Newtonian. Guiding cameras:Lodestar. Focal
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Object Name IC 2497 X-ray and Optical Images of IC 2497 New data from Chandra and other telescopes of a cosmic "blob" and a gas bubble could be a new way to probe the past activity of a giant black hole and its effect on its host galaxy. Hanny's Voorwerp, first discovered by a citizen scientist, is a gas cloud located next to the galaxy IC 2497. IC 2497 dropped in luminosity by at least 2 orders of magnitude in the last ∼105 yr. The system composed by HV and its galaxy is therefore a great laboratory to study AGN variability on previously inaccessible time-scales. The analysis of the galaxy allows us to study the present state of the AGN and the AGN-host galaxy inter- In the new study, researchers report that Hubble's cameras have uncovered star birth in a region of Hanny's Voorwerp that faces the spiral galaxy IC 2497, which is about 650 million light-years IC 2497 (također poznat kao IRAS 09380+3457 i PGC 165538) je spiralna galaksija koja je udaljena oko 692 miliona sg od Zemlje i nalazi se u sazviježđu Mali lav. Najveći prečnik je 0,60 (121 hiljada sg) a najmanji 0,3 uglovnih minuta (60 hiljada sg).
maja 1903. godine.[2][4][5] However, the nucleus of IC 2497 has very modest luminosity, with emission lines implying ionizing. luminosity < 10. 40 erg. s − 1. H I observations show that Hanny’s Voorwerp is a small part of a 300-kpc structure around the southern side of IC 2497 con taining 9 × 10. 9.
Top Message. A wide angle view of the patch of SDSS imaging containing "Hanny's Voorwerp", the blueish nebula next to galaxy IC 2497 at lower left of the image. IC 2497 Tag. Hanny's Voorwerp.
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Havolalar. IC 2497 Yangi umumiy katalog asl nashrida (ingl.); IC 2497 Yangi umumiy katalog asl nashrida (frans.) Query : IC 2497 C.D.S. - SIMBAD4 rel 1.7 - 2021.03.29CEST11:28:07 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations We demonstrate that Hanny’s Voorwerp is embedded ural weighting and a velocity resolution of 108 km s−1, and the in a large cloud complex of neutral hydrogen, possibly being the uniformly weighted 1.4-GHz continuum map.
Our WSRT continuum observations at 1.4 GHz and 4.9 GHz, reveal the presence of extended emission at the position of the nebulosity, although the bulk of the emission remains unresolved at the centre of the galaxy. e-VLBI 1.65 GHz
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A wide angle view of the patch of SDSS imaging containing "Hanny's Voorwerp", the blueish nebula next to galaxy IC 2497 at lower left of the image.
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