We owe our existence to stars, because they make the atoms of which we are formed. So if you are romantic you can say we are literally starstuff. If you're less romantic you can say we're the nuclear waste from the fuel that makes stars shine.
/ Sir Martin Rees /



In memoriam Halton C. Arp (1927-2013).


My astronomy sketches. Hover mouse over image for the inverted look. For fainter objects, take a look at the black-on-white original, sometimes it reveals more details.


Need advice? Want to discuss an observation? Feel free to contact me at flovro gmail*com.

ÚJ! Amennyiben elérhető, a ikonra kattintva magyarul is olvashatod az észlelést.


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By type: open clusters [67] globular clusters [14] diffuse nebulae [3] dark nebulae [0] planetary nebulae [27] variable stars [18] binary stars [23] asterisms [2] galaxies [119] quasars [1] planets [2] minor planets [1] comets [5] Sun [0] Moon [5] other objects [8]
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NGC 40 (Planetary nebula)
Also known as: Bow Tie Nebula
Right ascension: 0h 14m Declination: 72° 36'
Constellation: Cepheus
Date/time: 2012.09.11 23:30 UT
Equipment: 12" f/5 Newtonian
FoV: 7' Magnification and filter(s): 469x
Seeing: 7/10 Transparency: 3/5
SQM: 21.25 m/as2 Temperature: 11°C
Humidity: low Wind: none
Sight: 4 - lots of details, very interesting, unique look
Difficulty: 4 - hardly visible, dark adaptation and very dark skies needed, averted vision is required to see details
Position: 3 - moderate, some starhopping needed
Location: Nádasdladány, Hungary
Observer: Ferenc Lovró
Description:

A wonderful yet tiny little planetary. At small magnification (71x in my case) it looks like a slightly defocused star, however by increasing the power it soon starts to develop into a nice, perfectly round planetary nebula. Some details that also appea: to the South of the bright central star you may notice a small brighter blob, and to the West a bright feature can be seen that resembles a spiral arm of a galaxy. Doesn't react at all on UHC filter, but with an O-III it's size apparently grows, however the central star completely disappears, which is a bit weird, because the Westward star stays in the field even if it's fainter than the central star of the nebula. With low power it has a tint of purple-blue.


Hi-resolution image: [ reversed sketch | original sketch ]
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