martinsastro

Astronomy for all.

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Lester.jpg

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Logan


CRW_7538.jpg

4 files, last one added on Jan 07, 2012
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Centaurus_done.jpg
Centaurus_done.jpgCentaurus A.18 viewsThe Centaurus A/M83 Group is a complex group of galaxies in the constellations Hydra, Centaurus, and Virgo. The group may be roughly divided into two subgroups. The Cen A Subgroup, at a distance of 11.9 Mly (3.66 Mpc), is centered around Centaurus A, a nearby radio galaxy.[3] The M83 Subgroup, at a distance of 14.9 Mly (4.56 Mpc), is centered around the Messier 83 (M83), a face-on spiral galaxy.[3]

This group is sometimes identified as one group[4][5] and sometimes identified as two groups.[6] Hence, some references will refer to two objects named the Centaurus A Group and the M83 Group. However, the galaxies around Centaurus A and the galaxies around M83 are physically close to each other, and both subgroups appear not to be moving relative to each other.[3]

The Centaurus A/M83 Group is part of the Virgo Supercluster, the local supercluster of which the Local Group is an outlying member.
Martin
good.jpg
good.jpgNGC618818 viewsMartin
m42done.jpg
m42done.jpgM42.27 viewsThe Orion Nebula (also known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated south of Orion's Belt. It is one of the brightest nebulae, and is visible to the naked eye in the night sky. M42 is located at a distance of 1,344 ± 20 light years[2][5] and is the closest region of massive star formation to Earth. The M42 nebula is estimated to be 24 light years across. Older texts frequently referred to the Orion Nebula as the Great Nebula in Orion or the Great Orion Nebula.

The Orion Nebula is one of the most scrutinized and photographed objects in the night sky, and is among the most intensely studied celestial features.[6] The nebula has revealed much about the process of how stars and planetary systems are formed from collapsing clouds of gas and dust. Astronomers have directly observed protoplanetary disks, brown dwarfs, intense and turbulent motions of the gas, and the photo-ionizing effects of massive nearby stars in the nebula. There are also supersonic "bullets" of gas piercing the dense hydrogen clouds of the Orion Nebula. Each bullet is ten times the diameter of Pluto's orbit and tipped with iron atoms glowing bright blue. They were probably formed one thousand years ago from an unknown violent event.
Martin
Shane_Gilbert2.jpg
Shane_Gilbert2.jpg14 viewsMartin
Omegadone2G.jpg
Omegadone2G.jpgOmega Centaury.76 viewsJust testing the guiding on the G11 with Gemini 2Martin
test.jpg
test.jpg10 Minutes guiding test with the G11 Gemini2.53 viewsMartin
NGC253done2Meg.jpg
NGC253done2Meg.jpgNGC25352 viewsG11 guiding test on 24-08-2011 with latest August firmware.
10x200Sec RGB and 25x300Sec L on a ED80 and QHY9.
Uncropped.
Martin
NGC4945_supernova.jpg
NGC4945_supernova.jpgNGC494515 viewsNGC4945 with the supernova 2011ja (January 01-2012).Martin

Last additions
CentAfinal2G.jpg
CentAfinal2G.jpgCentaurus A5 views10 X 5 Min RGB and 15 X 10 Min Luminance.
MartinFeb 04, 2012
CRW_7538.jpg
CRW_7538.jpg12 viewsMartinJan 07, 2012
CRW_7537.jpg
CRW_7537.jpg9 viewsMartinJan 07, 2012
CRW_7536.jpg
CRW_7536.jpg11 viewsMartinJan 07, 2012
CRW_7535.jpg
CRW_7535.jpg10 viewsMartinJan 07, 2012
Eta_blue1Mb.jpg
Eta_blue1Mb.jpgEta Carinae19 views7X5 minute RGB and 7X10 minute LuminanceMartinJan 05, 2012
Eta_2Mb.jpg
Eta_2Mb.jpgEta Carinae.14 viewsFocused on the dimmest star without a Bahtinov mask worked better than with a mask.MartinJan 02, 2012
NGC4945_supernova.jpg
NGC4945_supernova.jpgNGC494515 viewsNGC4945 with the supernova 2011ja (January 01-2012).MartinJan 02, 2012