The Cepheid star RS Pup

The nebula around the Cepheid star RS Pup undoubtedly holds a wealth of information about the mass-loss history of this star. It will thus be instrumental to understand the evolution of Cepheids. Less than five years away from the centenary of the discovery of the Period-Luminosity relation by Leavitt & Pickering, RS Pup could well become a ''Rosetta stone'' for this important class of stars. This colour composite image is based on observations made with the 3.6-m ESO New Technology Telescope (NTT) installed at the La Silla Observatory (Chile) and equipped with the ESO Multi-Mode Instrument (EMMI). The image is based on data obtained through B, V, and R-filters. In order to avoid a heavy saturation of the detector, RS Pup was positioned in the gap between the detectors.

Mynd/Myndskeið:

ESO

Um myndina

Auðkenni:eso0805a
Tegund:Athuganir
Útgáfudagur:11. febrúar 2008
Tengdar fréttatilkynningar:eso0805
Stærð:1379 x 1376 px

Um fyrirbærið

Nafn:RS Puppis
Tegund:Milky Way : Star : Type : Variable
Fjarlægð:6500 ljósár
Constellation:Puppis
Flokkur:Nebulae

Myndasnið

Stór JPEG
261,4 KB

Bakgrunnsmynd

1024x768
168,9 KB
1280x1024
234,9 KB
1600x1200
284,7 KB
1920x1200
306,8 KB
2048x1536
389,4 KB

Hnit

Position (RA):8 13 4.17
Position (Dec):-34° 34' 43.24"
Field of view:5.72 x 5.70 arcminutes
Stefna:Norður er 120.2° højre frá lóðréttu

Litir og síur

TíðnisviðSjónauki
Sýnilegt
B
New Technology Telescope
EMMI
Sýnilegt
V
New Technology Telescope
EMMI
Sýnilegt
R
New Technology Telescope
EMMI

 

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