Uwe Glahn
September 20th, 2015, 07:01 PM
IC 1311 (Cr 414, Lund 928, C 2008+410, Tr 36)
R.A.: 20h10m47s
Dec.: +41°10'19"
Size: 5.0'
Type: I 1 r n
Total mag (V): 13.1
SB (V) 16.6
Number of stars: 60
Mag of brightest star (V): 17.0
The northern Milky Way is full of interesting open clusters. One of the highlights and my personal favorite of all is IC 1311.
With 2.3° (WNW) distance to Sadr (gamma Cyg) the cluster stands high in the sky, also for northern observers and can be observed for several summer – autumn months. Although good placed in the sky, the finding is a little bit tricky because of the lots of stars in the region – maybe the reason of its anonymous status.
The physical parameters of this old cluster are often examined but still not very precise. The distance ranges between 5kpc – 16kpc and the age between 0.8Gys and 2Gys. More important for us are the I 1 r n Trumpler type (strong concentration, most stars of nearly the same brightness, rich, cluster in involved in nebulosity) and the number of stars. More about the magnitudes later.
When we look deeper in the photographs of Rosso (http://www.renzodelrosso.com/profondocielo/foto/deep/digitale/ammassi/foto/ic1311_2011.jpg) or with bigger aperture of the 4m-Mayall (https://www.noao.edu/image_gallery/html/im1250.html) telescope, the surrounding of the cluster looks like shells of a large PN. The Capella-team (http://www.capella-observatory.com/images/DiffuseNebula/IC1311Vergleich.jpg) made Ha and [OIII] exposures which shows, that a PN is very unlikely.
When it comes to the practical observation the SB and the faint magnitude of the brightest star act as a deterrent but in reality the cluster can bee seen under good transparency with a 4" telescope. The brighter stars which frames the cluster stands out first – that is why I call it "crowned". From 8" the cluster began to show a mottled structure. With 27" the cluster is fully resolved into dozens of stars. In contrast to the Trumpler classification the visible concentration is not so distinct.
Beside the open cluster itself the neighborhood offers lots of types of objects like the small and faint PN K 4-51 (PNG 077.7+03.7, 25' SE), the poor OC Dolidze 2 (16' NW) or the DN B 342 (16' W).
Martin Germano, 8"
1790
As always, give it a go and let us know!
R.A.: 20h10m47s
Dec.: +41°10'19"
Size: 5.0'
Type: I 1 r n
Total mag (V): 13.1
SB (V) 16.6
Number of stars: 60
Mag of brightest star (V): 17.0
The northern Milky Way is full of interesting open clusters. One of the highlights and my personal favorite of all is IC 1311.
With 2.3° (WNW) distance to Sadr (gamma Cyg) the cluster stands high in the sky, also for northern observers and can be observed for several summer – autumn months. Although good placed in the sky, the finding is a little bit tricky because of the lots of stars in the region – maybe the reason of its anonymous status.
The physical parameters of this old cluster are often examined but still not very precise. The distance ranges between 5kpc – 16kpc and the age between 0.8Gys and 2Gys. More important for us are the I 1 r n Trumpler type (strong concentration, most stars of nearly the same brightness, rich, cluster in involved in nebulosity) and the number of stars. More about the magnitudes later.
When we look deeper in the photographs of Rosso (http://www.renzodelrosso.com/profondocielo/foto/deep/digitale/ammassi/foto/ic1311_2011.jpg) or with bigger aperture of the 4m-Mayall (https://www.noao.edu/image_gallery/html/im1250.html) telescope, the surrounding of the cluster looks like shells of a large PN. The Capella-team (http://www.capella-observatory.com/images/DiffuseNebula/IC1311Vergleich.jpg) made Ha and [OIII] exposures which shows, that a PN is very unlikely.
When it comes to the practical observation the SB and the faint magnitude of the brightest star act as a deterrent but in reality the cluster can bee seen under good transparency with a 4" telescope. The brighter stars which frames the cluster stands out first – that is why I call it "crowned". From 8" the cluster began to show a mottled structure. With 27" the cluster is fully resolved into dozens of stars. In contrast to the Trumpler classification the visible concentration is not so distinct.
Beside the open cluster itself the neighborhood offers lots of types of objects like the small and faint PN K 4-51 (PNG 077.7+03.7, 25' SE), the poor OC Dolidze 2 (16' NW) or the DN B 342 (16' W).
Martin Germano, 8"
1790
As always, give it a go and let us know!