View allAll Photos Tagged 247:
247 903-8 mit dem GM 60006 bei der Durchfahrt von Baalberge
247 903-8 power's her train through Baalberge
26.05.2017
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MÁV 424 247 depart Tapolca with passenger train (19747) Tapolca to Balatonfüred service on 05.07.2020.
ECR/DB 247 056 - 56522 (Wacker Werke [Burghausen] - Mühldorf) / Metrans 761 007 - Tüßling - 12.07.2013
Hungarian steam loco MÁV Class 424 No.424.247 is seen passing Szepezdfürdő with the express no.1973 Tapolca to Balatonfüred during the Hungary Balaton Retro Weekend.
The MÁV 424's working was a every day passenger train thats normally worked by a 418 diesel.
Taken on the 6th July 2024.
A double traction 186 247 (and ES 64 F4-027) leads "EKOL" train to Tarvisio Boscoverde near Pöckau station on 27.02.2015.
193 247 mit RE 10 (95902)von Tübingen nach Heilbronn.(Metzingen(Württ.)ehem.Bahnhposten 31 18.6.2020).
Vojkovice nad Svratkou,
"Plechacz" z pociągiem osobowym 4609 ze stacji Křižanov do stacji Hustopeče u Brna zbliża się do miejscowego przystanku osobowego. Niestety w roku 2023 nastąpił kres eksploatacji lokomotyw serii 242 w Brnie. Została sporadyczna obsługa "osobówek" w trybie awaryjnym oraz pojedyncze połączenie na zasadzie obiegów uzupełniających. Dotychczasowe obiegi "Plechaczy" zostały przejęte przez elektryczne jednostki tracyjne serii 530 i 550, które stały się podstawową serią do połączeń osobowych eksploatowaną przez Brno-Maloměřice.
Machine 749 247-3 took over the 2nd year of Retro Express Slovakia. On the trail, it climbs towards the Besnícky tunnel and passes the abandoned Vernár station.
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247 904-6 von DB Cargo neben dem Stellwerk W1 in Bernburg
247 904-6 of DB Cargo next to the switch tower W1 of Bernburg
21.02.2017
"My sister said, You're making it hard for all us housewives in Nebraska." ~Kate Millett
Meet Liza… Bartender/Manager in Austin, originally from Nebraska… Hence her "corn-husker" on her left arm… Another addition to the tattoo series (I have 4 more left) of the project. Don't let the innocent look fool you. She's as crazy as I am…!! hahahaha….Thanks mama.
Strobists:
SB600 camera front right 6ft from background interfit grid 1/8 @85mm
AB800 camera front boomed 4ft on axis from Liza in beauty dish with sock @1/8
1/200 @F/10
ISO 200
Nikon 80-200 2.8
Triggered with Cybersync
see setup
247 038 kommt mit dem "Wackershuttle" aus dem Wackerwerk in Burghausen und wird den Zug zusammen mit einer Schwestermaschine am Zugschluss nach Landshut befördern, wo dann eine E-Lok die Traktion übernehmen wird. Hier zeigte sich der Zug bei Heiligenstatt dem Fotografen.
A Chinook helicopter carries 2600 gallons of water to the fire on Teepee Mountain in northwest Montana. Two of these incredible units used my cabin as a turning point on their mission. I just watched in wonder...
This Hubble image shows the central region of a spiral galaxy known as NGC 247. NGC 247 is a relatively small spiral galaxy in the southern constellation of Cetus (The Whale). Lying at a distance of around 11 million light-years from us, it forms part of the Sculptor Group, a loose collection of galaxies that also contains the more famous NGC 253 (otherwise known as the Sculptor Galaxy).
NGC 247’s nucleus is visible here as a bright, whitish patch, surrounded by a mixture of stars, gas and dust. The dust forms dark patches and filaments that are silhouetted against the background of stars, while the gas has formed into bright knots known as H II regions, mostly scattered throughout the galaxy’s arms and outer areas.
This galaxy displays one particularly unusual and mysterious feature — it is not visible in this image, but can be seen clearly in wider views of the galaxy, such as a picture from ESO’s MPG/ESO 2.2-meter telescope. The northern part of NGC 247’s disc hosts an apparent void, a gap in the usual swarm of stars and H II regions that spans almost a third of the galaxy’s total length.
There are stars within this void, but they are quite different from those around it. They are significantly older, and as a result much fainter and redder. This indicates that the star formation taking place across most of the galaxy’s disk has somehow been arrested in the void region, and has not taken place for around one billion years. Although astronomers are still unsure how the void formed, recent studies suggest it might have been caused by gravitational interactions with part of another galaxy.
Image Credit: NASA/ESA