Van den Bergh 130 is a small reflection nebula in Cygnus located in an interesting field full of different nebulae immediately southwest of the 2^nd magnitude star γ Cygni (Sadr). The field also contains emission nebulae like Sharpless 108, dark nebulae like Barnard 343 and Barnard 344 and other reflection nebulae like GM 2-39.

I have created this bicolor image using exposures taken with Hα and [OIII] narrowband filters on my 4.9" Wright-Newtonian, 6" Newtonian and 2.8" refractor telescopes. All exposures were taken in my backyard in Vienna, Austria during 8 nights in the summer of 2022. Single-shot color exposures were added for the star colors. The nebulae are labelled in a mouse-over of the color image.

An image of the Heart Nebula IC 1805, which is an emission nebula located in the constellation Cassiopeia, five degrees north of the famous Double Cluster in Perseus. The nebula is composed of glowing gas and dust, illuminated by young, hot stars, many of which are members of the star cluster Melotte 15, which is nestled within the nebula. Follow the link to see a 100% enlargement of the nebula's center and of the area around the Planetary Nebula PN G135.6+01.0 (WeBo 1), which is located at the eastern edge of IC 1805.

This is a bicolor image taken with Hα and [OIII] narrowband filters on my 4.9" Wright-Newtonian and 6" Newtonian telescopes. All exposures were taken in my backyard in Vienna, Austria during six January nights. Star colors were taken from an older DSLR image of the same nebula.

Another famous supernova remnant (SNR) is IC 443 the Jellyfish Nebula in the constellation Gemini. I have taken a wide-field image of this SNR which is framed by the 3^rd magnitude stars μ and η Geminorum. The image also contains the older SNR G189.6+3.3, the emission nebula Sh2-249 and the mixed emission/reflection nebula IC 444.

This is a bicolor Hα/[OIII] image taken with narrowband filters; star colors were added from separate color images. I used my 3-telescope "Triplet" setup for this image: The 4.9" Wright-Newtonian and the 6" Newtonian for Hα and [OIII] and the 2.8" refractor for star colors. All exposures were taken in my backyard in Vienna, Austria in March 2023 and January 2024.

An image of NGC 6960/74/79, the Western Veil and Pickering's Triangle in Cygnus. The Veil Nebula is the remnant of massive star, which exploded 10,000-20,000 years ago in a supernova.

The nebulosity emits all of its light in isolated emission lines. The most prominent of those are the Hα, [OIII] and [SII] lines, which I recorded with narrowband filters to create the color image. This is a "natural color" composition mixed so that the resulting colors are close to the visible spectrum of the human eye. For the star colors I used a color photo of the same nebula taken in 2006 with a Canon DSLR camera. For all images I used the 4.9" Wright-Newtonian telescope. All exposures were taken in my backyard in Vienna, Austria in 6 different nights in August 2013 and October 2021. The total exposure time amounts to 22.8 hours for the narrowband data.

An image of NGC 6888, the Crescent Nebula and its western surroundings in Cygnus. The Crescent Nebula was formed by fast stellar wind from the Wolf-Rayet star WR 136 colliding with slower moving stellar wind from an earlier stage of the same star. The background is dominated by red-colored HII nebulae which cover large parts of the constellation.

This is a bicolor Hα/[OIII] image taken with narrowband filters; star colors were added from separate color images. I used my 3-telescope "Triplet" setup for this image: The 4.9" Wright-Newtonian for Hα, the 6" Newtonian for [OIII] and the 2.8" refractor for star colors. All exposures were taken in my backyard in Vienna, Austria in the Autumn of 2022.

New processing of the image of Sharpless 126. The broadband images were taken during my stay at the Großglockner-Hochalpenstraße in September 2020, the narrowband images (Hα and [OIII]) in Vienna. This is an interesting region in southern Lacerta, where a blue-green molecular cloud (LBN 437) overlaps with a large red emission nebula (Sh2-126), forming a "stellar funnel" containing a symmetric reflection nebula. The total exposure time is 30 hours: 9 hours under dark mountain skies for broadband color, 10 hours for narrowband Hα and 11 hours for narrowband [OIII]. All images were taken with the 125 mm Wright-Newtonian. The color images taken in the mountains have a much better depth than the narrowband images taken in Vienna. Processing the Hα and especially the [OIII] images was difficult, mainly because of the uneven gradients in the city sky.

Astronomy in the City: In the late summer of 2021, I took exposures of the Tulip Nebula (Sh2-101) in Cygnus from my backyard in Vienna, Austria using Hα and [OIII] narrow-band filters with good results. I mixed the two monochrome images for a near-natural color image. The Hα image also turned out surprisingly well for a light-polluted city sky. I used the 9.5" Newtonian reflector and a ZWO ASI1600MM Pro monochrome camera for the exposures. I have added starless version of both images as mouse-overs.

A telelens photograph of IC 5146 - Cocoon Nebula and Surrounding Area, which is located in a dense part of the Milky Way in Northern Cygnus. It can be found at the eastern end of the elongated dark cloud Barnard 168 and is part of an extended molecular cloud. An annotated version of the image is overlaid on mouse-over or touch. This photo was taken parallel to the telescope image below. The Samyang 135mm lens was used mounted piggy-back on the main telescope.

During my August 2023 stay in the Austrian Alps I had the fortune to enjoy three clear nights in a row, two of which I used to get a deep image of IC 5146, the Cocoon Nebula and the prominent large dark nebula Barnard 168 running towards it from the northwest. For this exposure series, I used my I used my 3-telescope "Triple Setup" and 3 cameras to capture color, Hα and [OIII] images at the same time.

During the 2023 Perseid meteor shower, I have only been able to go out to a dark observation site during the night of August 14-15, when the meteor activity was on its decline. However, I got lucky and captured a moderately bright Perseid streaking down along the Summer Milky Way, changing color and emitting a small flash towards the end of its trail. The camera used was my trusty old Nikon D7000, the exposure time 20 seconds, and the focal length 18mm at f/3.5. The camera was mounted on a fixed tripod. I was actually taking a timelapse exposure series, and this is one of the images.

I have updated the Telescopes and Equipment page and included pictures of all telescopes and most cameras which I currently use. This page is, of course, subject to frequent changes, although I tend to keep my trusty equipment for a long time. I generally try to master all of my equipment and reach the best performance it can offer before moving on, and this takes years.

Sh2-150 in Cepheus is a red emission nebula with a blue relection nebula (vdB 154) on top. For the emission nebula, the narrow-band Hα filter was used in my backyard in Vienna, Austria. The reflection nebula, on the other hand, required dark skies, which I found at the Steyersberger Schwaig in Lower Austria. All exposures were taken by my 125mm Wright-Newtonian reflector. See also the Hα image for high contrast detail within the emission nebula.

A short animation of the "Green Comet" C/2022 E3 (ZTF) (YouTube link) consisting of 56 images and showing the comet's quite rapid movement during 3 hours. The autoguider was trained on the comet's core. Moonlight, bad seeing & light-polluted sky somewhat degraded the images. I used my 150mm f/4 Newtonian for these exposures, which were taken in my backyard in Vienna, Austria.

The exposures for this image of the Propeller Nebula in Cygnus were taken during the summers of 2019, 2020 and 2022. Interestingly, astronomers do not know much about this peculiar structure, even its distance from Earth is undetermined. I used by trusty old 125mm Wright-Newtonian, several CCD/CMOS cameras and a set of narrow-band Hα and [OIII] filters for this image. Single-shot color exposures taken at the Steyersberger Schwaig (a relatively dark site in the Austrian Alps) were mixed in mainly for the colors of the stars. See also the Hα image for high contrast detail within the nebula. I have removed the stars in a mouse-over of each image.

A telelens photograph of Cepheus Center - Wolf's Cave Nebula and Environment, which is located in Cepheus, in the Milky Way. Nearly all of the image is filled with nebulae. An annotated version of the image is overlaid on mouse-over or touch. This photo was taken during my stay at the Postalm in September 2022. The Samyang 135mm lens was used mounted piggy-back on the main telescope.

This image of van den Bergh 152 - Wolf's Cave Nebula and its surrounding area was taken using a "Triple Setup" of telescopes: A 154mm Newtonian for one-shot color, a 125mm Wright-Newtonian for Hα narrowband and a 72 refractor for [OIII] narrow-band exposures. All were mounted side-by-side on my EQ6-R equatorial mount and guided using a small guidescope. It took three nights with the Triple Setup to acquire enough data for this image. One of the nights fell into my stay at the Postalm in September 2022. As usual, I have removed the stars in a mouse-over.

My September 2022 astrophotography excursion again led me to the Postalm, an alpine pasture located in the Salzkammergut, in Salzburg, at a height of about 1300m. However, I had but one night suited for astrophotography and was further hindered by light pollution and moisture. Read my report about this astro-expedition (in German), which will soon be amended with astrophotos.

WR 134 - Wolf-Rayet Bubble in Cygnus was another long-term project which took me 9 nights to complete from September 2020 to August 2022. I invested about 30 hours of total exposure time in these images using my 125mm Wright-Newtonian and Hα and [OIII] narrow-band filters in my light-polluted backyard in Vienna. I also took single-shot color exposures under dark mountain skies to capture the colors of the stars. All of those exposures were combined in the color image. I have also uploaded the Hα and [OIII] greyscale images for comparison. As a bonus I have removed the stars in a mouse-over of each image. Note the delicate structure of the bubble best seen in the starless images!