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Serpens star forming region
The figure shows the Serpens star-forming region, as it was imaged during commissioning, on HAWK-I's four large infrared detectors. The gap between them is real, and multiple exposures are required to make a filled-in picture. The colour composite was created from images taken through three filters, J, H and K.
Kredit:ESO
O snímku
| Id: | eso0736b |
| Typ: | Pozorování |
| Datum zveřejnění: | 22. srpna 2007 |
| Související články: | eso0736 |
| Velikost: | 4244 x 4236 px |
O objektu
| Jméno: | Serpens Nebula |
| Typ: | Milky Way : Nebula : Appearance : Dark Milky Way : Nebula : Appearance : Reflection |
| Vzdálenost: | 1000 světelné roky |
| Constellation: | Serpens Cauda |
| Kategorie: | Nebulae |
Image Formats
Souřadnice
| Position (RA): | 18 29 55.43 |
| Position (Dec): | 1° 17' 11.54" |
| Field of view: | 7.52 x 7.51 arcminutes |
| Orientace: | Sever je 0.0° levá od svislé osy |
Zobrazit ve World Wide Telescope:
Barvy & filtry
| Pásmo | Dalekohled |
|---|---|
| Infračervený J | Very Large Telescope HAWK-I |
| Infračervený H | Very Large Telescope HAWK-I |
| Infračervený K | Very Large Telescope HAWK-I |