Dumbbel Nebula M27

The Dumbbell Nebula (also known as Messier 27, M 27, or NGC 6853) is a planetary nebula (PN) in the constellation Vulpecula, at a distance of about 1,360 light years.
This object was the first planetary nebula to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and its diameter of about 8 arcminutes, it is easily visible in binoculars, and a popular observing target in amateur telescopes.

Instruments and exposure data:

W.O FLT110 with dedicated TMB field flattener
FeatherTouch 3'' focuser
Starizona MicroTouch autofocuser
W.O ZS80 ED
SBIG ST10XME CFW9
Meade DSI
Filters: Ha 5nm Astrodon_RGB Baader Planetarium
Sky-Watcher EQ6 Pro

L(Ha+Red)_Red(Ha+Red+Red)_Green_Blue

Ha:10*5min bin1x1_46*10min bin1x1
Red:28*4min bin1x1
Green:29*4min bin1x1
Blue:25*4min bin1x1
Total exposure time:13h58min

For full resolution please see in Astrobin

NGC 7635: THE BUBBLE NEBULA

NGC 7635, also called the Bubble Nebula and Sharpless 162, is a H II region[2] emission nebula in the constellation Cassiopeia. It lies close to the direction of the open cluster Messier 52. The "bubble" is created by the stellar wind from a massive hot, 8.7[2] magnitude young central star, the 15 ± 5 M☉[4] SAO 20575 (BD+60 2522).[7] The nebula is near a giant molecular cloud which contains the expansion of the bubble nebula while itself being excited by the hot central star, causing it to glow.[7] It was discovered in 1787 by Friedrich Wilhelm Herschel.[6] The star SAO 20575 or BD+602522 is thought to have a mass of 10-40 Solar masses.

Tricolor Emission Line Image


Instruments and exposure data:

W.O FLT110 with dedicated TMB field flattener
FeatherTouch 3'' focuser
Starizona MicroTouch autofocuser
W.O ZS80 ED
SBIG ST10XME CFW9
Meade DSI
Filters:
SII 8nm Baader Planetarium
Ha 5nm Astrodon
OIII 8.5nm Baader Planetarium

Sky-Watcher EQ6 Pro

SII :26*10min bin1x1
Ha :20*10min bin1x1
OIII:24*10min bin1x1

Total exposure time:11h40min

SH 2 171 modified Hubble palette _ reworked

Cosmic pillars of cold molecular gas and clouds of dark dust lie within Sharpless 171, a star-forming region some 3,000 light-years away in the royal constellation Cepheus. This tantalizing false-color skyscape spans about 20 light-years across the nebula's bright central region. It also highlights the pervasive glow of emission from atomic gas using narrowband filters and a color palette made popular in Hubble Space Telescope images. Powering the nebular glow are the young, hot stars of a newly formed cluster, Berkeley 59. Of course, this star-forming region is entry number 171 in the famous 1959 catalog of emission nebulae compiled by astronomer Stewart Sharpless.

explanation from : NASA apod 2008 October

Tricolor Emission Line Image

Instruments and exposure data:

W.O FLT110 with dedicated TMB field flattener
FeatherTouch 3'' focuser
Starizona MicroTouch autofocuser
W.O ZS80 ED
SBIG ST10XME CFW9
Meade DSI
Filters:
SII 8nm Baader Planetarium
Ha 5nm Astrodon
OIII 8.5nm Baader Planetarium

Sky-Watcher EQ6 Pro

SII :30*15min bin1x1
Ha :30*15min bin1x1
OIII:30*15min bin1x1

Total exposure time:22h30min

Elephant's Trunk nebula IC1396 _ rework

Instruments and exposure data:

W.O FLT110 with dedicated TMB field flattener
FeatherTouch 3'' focuser
Starizona MicroTouch autofocuser
W.O ZS80 ED
SBIG ST10XME CFW9
Meade DSI

Sky-Watcher EQ6 Pro

Tricolor Emmision Line image
S[II] 8nm(Red)_Ha 5nm(Green)_O[III] 3nm(Blue)
Modified Hubble Palette

S[II] 25*15min_Ha 29*15min_O[III] 18*15min
total exposure time : 1080min (18h)

The Elephant's Trunk nebula is a concentration of interstellar gas and dust in the star cluster IC 1396 – an ionized gas region located in the constellation Cepheus about 2,400 light years away from Earth.[1] The piece of the nebula shown here is the dark, dense globule IC 1396A; it is commonly called the Elephant's Trunk nebula because of its appearance at visible light wavelengths, where there is a dark patch with a bright, sinuous rim. The bright rim is the surface of the dense cloud that is being illuminated and ionized by a very bright, massive star that is just to the west of IC 1396A.The entire IC 1396 region is ionized by the massive star, except for dense globules that can protect themselves from the star's harsh ultraviolet rays.

The Elephant's Trunk nebula is now thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards of stars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity.

The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk nebula. This pressure has triggered the current generation of protostars.[2]

Melotte 15 in IC1805

Tricolor Emmision Line image
S[II] 8nm(Red)_Ha 5nm(Green)_O[III] 3nm(Blue)
Modified Hubble Palette

Instruments and exposure data:

S[II] 22*15min_Ha 39*10min_O[III] 26*15min
total exposure time : 1110min (18h 30min)

W.O FLT110 with dedicated TMB field flattener

FeatherTouch 3'' focuser
Starizona MicroTouch autofocuser
W.O ZS80 ED
SBIG ST10XME CFW9
Meade DSI
Sky-Watcher EQ6 Pro

Filters:
Ha 5nm Astrodon

S[II] 8nm Baader

O[III] 3nm Astrodon

Kallithea Athens Hellas

Anacortes Image of the Day 22/11/2011

Elephant's Trunk nebula IC1396

Tricolor Emmision Line image
S[II] 8nm(Red)_Ha 5nm(Green)_O[III] 3nm(Blue)
Modified Hubble Palette

S[II] 25*15min_Ha 29*15min_O[III] 18*15min
total exposure time : 1080min (18h)

Τελικά δεν άντεξα...και πήρα το 3nm O[III] .
Αν και βινιετάρει περισσότερο(μικρό το κακό) από αυτό της Baader , πέτυχα σημαντικά καλύτερο S/N!!!
Kallithea Athens Hellas

Anacortes Image of the Day 3/10/2011

Sharpless 171 Hubble palette

Tricolor Emission Line Image

Instruments and exposure data:

W.O FLT110 with dedicated TMB field flattener

FeatherTouch 3'' focuser

Starizona MicroTouch autofocuser

W.O ZS80 ED
SBIG ST10XME CFW9
Meade DSI 

Filters:

SII 8nm Baader Planetarium

Ha 5nm Astrodon

OIII 8.5nm Baader Planetarium

Sky-Watcher   EQ6 Pro

SII :30*15min bin1x1
Ha :30*15min bin1x1

OIII:30*15min bin1x1

Total exposure time:22h30min 

Anacortes Image of the Day 19/09/2011

Northern Galactic Image of the Month Award for September 2011

http://www.northerngalactic.com/forum/news.php

NGC 7331 and Stephan's quintet

                                       

The spiral galaxy NGC 7331, in Pegasus, can be seen with small telescopes under dark skies as a faint fuzzy spot. It is an island universe similar to our own Galaxy (or maybe somewhat larger) and placed at a distance of 50 million light-years. NGC 7331 was discovered by Wilhelm Herschel in 1784

Stephan's Quintet in the constellation Pegasus is the first identified compact galaxy group of five galaxies about 300 million light-years away. The group was discovered by Édouard Stephan in 1877 at Marseilles Observatory. The group is the most studied of all the compact galaxy groups.

Recent infrared observations made with NASA's Spitzer Space Telescope have revealed the presence of a huge intergalactic shock wave, or "sonic boom" in the middle of Stephan's Quintet. This discovery, made by an international research team including scientists from the Max Planck Institute for Nuclear Physics (MPIK) in Heidelberg, provides a local view of what might have been going on in the early universe, when vast mergers and collisions between galaxies were commonplace.

Instruments and exposure data

W.O FLT110 with dedicated TMB field flattener and Feather Touch 3'' focuser

SBIG ST10XME CFW9

Starizona MicroTouch autofocuser

EQ6

Baader RGB filters

Luminance: 74*8min(bin1x1) total 9h52min

21-22/8/2010_17-19/9/2010

Red: 11*5min(bin1x1) Green: 11x5min(bin1x1) Blue: 18x5min(bin1x1) total 3h20min

FWHM: 3.41’’-4.89’’ 

Kallithea Athens Hellas

Aφιερωμένη στον αγαπητό μου φίλο Γιάννη Ελευθεριάδη!!!

Γιάννη άργησα 2 μήνες αλλά πιστεύω το αποτέλεσμα να σου αρέσει...
Anacortes Image of the  Day 3-10-2010                                                     

(Sh2-101) Sharpless 2-101, an emission nebula in Cygnus

(Sh2-101) Sharpless 2-101, an emission nebula in Cygnus.
Sh2-101 also known as Tulip Nebula, is a quite bright emission nebula.

W.O FLT110 with dedicated TMB field flattener and Feather Touch 3'' focuser
SBIG ST10XME CFW9
Starizona MicroTouch autofocuser
EQ6
Astrodon 5nmHα
240 min _30*8min subs

Anacortes Image of the Day 14-06-2010

NGC 7635 Bubble Nebula Hubble palette

full resolution

60% of the original size

NGC 7635, also called the Bubble Nebula and Sharpless 162, is a H II region[2] emission nebula in the constellation Cassiopeia. It lies close to the direction of the open cluster Messier 52. The "bubble" is created by the stellar wind from a massive hot, 8.7[2] magnitude young central star, the 15 ± 5 M☉[4] SAO 20575 (BD+60 2522).[7] The nebula is near a giant molecular cloud which contains the expansion of the bubble nebula while itself being excited by the hot central star, causing it to glow.[7] It was discovered in 1787 by Friedrich Wilhelm Herschel.[6] The star SAO 20575 or BD+602522 is thought to have a mass of 10-40 Solar masses.
W.O FLT-110 with dedicated field flattener
EQ6 Pro
ST10XME
Astrodon 5nm Ha filter
Baader 8nm SII filter
Baader 8.5nm OIII filter
Ha: 3h 20min
SII: 4h 20min
OIII:4h
Total exposure 11h40min under near full moon from Kallithea Athens Greece.
Anacortes Image of the Day 08/09/2009

M27 , the Dumbbell Nebula in Hydrogen Alpha Light

invert

68% of full resolution

Full resolution

EQ6,FLT110,ST10XME Ha 5nm 8,5 hours exposure.
The Dumbbell Nebula (also known as Messier 27, M 27, or NGC 6853) is a planetary nebula (PN) in the constellation Vulpecula, at a distance of about 1,360 light years.
This object was the first planetary nebula to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and its diameter of about 8 arcminutes, it is easily visible in binoculars, and a popular observing target in amateur telescopes.
Τελικά κατάφερα να μαζέψω τα φωτόνια που ήθελα....με τη βοήθεια του Φεγγαριού μάζεψα λίγα παραπάνω ,αλλά τι να κάνεις αυτά έχει η ζωή...!
EQ6 EQMOD FLT110 TMB FF ST10XME .
510 λεπτά (10x5min + 46x10min) στο 5nm Ηα της Astrodon ή 8,5 ώρες σε 4 νύχτες στη διάρκεια 2 εβδομάδων!!!
Όλη η επεξεργασία έγινε αποκλειστικά στο CCDStack με μια μικρή επέμβαση στα curves στο PS.
Αποθορυβοποίηση με 33% ΝoiseNinja
Καμία αισθητική ή άλλου είδους επέμβαση στα άστρα.
Την 1η νύχτα από λάθος η κάμερα ήταν τοποθετημένη 90 μοίρες clockwise...για αυτό και έχει γίνει crop στην κεντρική περιοχή .
Anacortes Image of the Day 07/26/2009

Mars

Mars 01/11/2008 21:41 UTC
Distance from Earth 0.65au
Illumination 98%
Angular diameter 14.4arcsec CM 27
8'' LX90 f/25
x2.5 PowerMate
Baader Ir-cut
DBK 21AF04
Kallithea
Athens
Hellas

http://www.buytelescopes.com/viewphoto.aspx?pid=16455