Eclipsing binary system in Orion

The RXJ 0529.4+0041 system after primary eclipse. The object RXJ 0529.4+0041 was first discovered by the X-ray satellite ROSAT. Subsequent optical spectroscopy showed this object to be a young, low-mass spectroscopic binary system. And when a team of astronomers used a 91-cm telescope at the Serra La Nave observing station on the slope of the Etna volcano (Sicily) to monitor the light curve, they also discovered that this system undergoes eclipses.


This is one of the six individual frames from the ADONIS movie of the RXJ 0529.4+0041 eclipsing, binary stellar system, corresponding to the time around the "primary" eclipse. 

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ESO

Om bilden

ID:eso0133c
Typ:Observation
Publiceringsdatum:8 oktober 2001
Relaterade pressmeddelanden:eso0133
Storlek:727 x 641 px

Om objektet

Namn:RXJ 0529.4+0041
Typ:Milky Way : Star : Grouping : Binary
Avstånd:1400 ljusår
Kategori:Stars

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Originalstorlek
242,4 kB
Stor jpeg
109,0 kB
Skärmstor jpeg
140,8 kB

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Färger och filter

BandTeleskop
Infrarött
K
ESO 3.6-metre telescope
ADONIS
Infrarött
H
ESO 3.6-metre telescope
ADONIS
Infrarött
J
ESO 3.6-metre telescope
ADONIS