Images

Omega Centauri with the NTT ESO-MPE-MPA-USM-Workshop Charon's Occultation on July 11, 2005 Radial Velocity Curve of Gliese 581 (HARPS/3.6m)
Omega Centauri with the NTT ESO-MPE-MPA-USM-Workshop Charon's Occultation on July 11, 2005 Radial Velocity Curve of Gliese 581 (HARPS/3.6m)
Spectral Energy Distribution of GRB 050904 Light curves of the black-hole GU Muscae Computerworld Honors Program 21st Century Achievement Award  Positions of 2M1207A and of its Companion
Spectral Energy Distribution of GRB 050904 Light curves of the black-hole GU Muscae Computerworld Honors Program 21st Century Achievement Award Positions of 2M1207A and of its Companion
Colour-Magnitude Diagram of 2341 Stars towards N214C Spectrum of the Companion of GQ Lupi Observed Separation between GQ Lupi and its Companion Properties of Young Massive Clusters
Colour-Magnitude Diagram of 2341 Stars towards N214C Spectrum of the Companion of GQ Lupi Observed Separation between GQ Lupi and its Companion Properties of Young Massive Clusters
The Double Main Sequence of Omega Centauri Average Spectra of the Blue and Red Population Stars Brightness "Dip" and Velocity Variations of OGLE-TR-122 Spectrum of Two Regions on Titan
The Double Main Sequence of Omega Centauri Average Spectra of the Blue and Red Population Stars Brightness "Dip" and Velocity Variations of OGLE-TR-122 Spectrum of Two Regions on Titan
Mid-IR spectra of Comets and Protoplanetary Discs Mid-IR spectra of HD 142527 Inner Disc and Common Dust Types Period-Luminosity relation for Cepheids Pulsation of the Cepheid Variable L Car
Mid-IR spectra of Comets and Protoplanetary Discs Mid-IR spectra of HD 142527 Inner Disc and Common Dust Types Period-Luminosity relation for Cepheids Pulsation of the Cepheid Variable L Car
"Velocity Curve" of mu Arae Velocity Variation of mu Arae Observed by HARPS Details of the Meteor Spectrum (FORS1/VLT) Optical Spectrum of the Bipolar Nebula
"Velocity Curve" of mu Arae Velocity Variation of mu Arae Observed by HARPS Details of the Meteor Spectrum (FORS1/VLT) Optical Spectrum of the Bipolar Nebula
Velocity Variations Caused by Two Transiting Exoplanets Relative Changes with Redshift of the Fine Structure Constant Zoom-in on a Possible Cluster of Galaxies (in box) XMM-Newton Contour Map Overlaid on a CFHT I-band image
Velocity Variations Caused by Two Transiting Exoplanets Relative Changes with Redshift of the Fine Structure Constant Zoom-in on a Possible Cluster of Galaxies (in box) XMM-Newton Contour Map Overlaid on a CFHT I-band image
Spectra of Virgo Intracluster HII region Lyman-alpha Forest in QSO HE2217-2818 Mass Function of Globular Clusters Observations of Comet Hale-Bopp from La Silla
Spectra of Virgo Intracluster HII region Lyman-alpha Forest in QSO HE2217-2818 Mass Function of Globular Clusters Observations of Comet Hale-Bopp from La Silla
Observations of Comet Hale-Bopp from La Silla Minor Planet (4015) / Comet Wilson–Harrington The lightcurve of Supernova 1987A The VLT Adaptive Optics Prototype System
Observations of Comet Hale-Bopp from La Silla Minor Planet (4015) / Comet Wilson–Harrington The lightcurve of Supernova 1987A The VLT Adaptive Optics Prototype System
Deneb observed with the VLT Adaptive Optics Prototype System The large jet in the HH-111 complex Eclipse of Pluto on April 2, 1986 Screenshot from ESO Video News Release 43 (B-roll)
Deneb observed with the VLT Adaptive Optics Prototype System The large jet in the HH-111 complex Eclipse of Pluto on April 2, 1986 Screenshot from ESO Video News Release 43 (B-roll)
Aerial view of ESO's Headquarters Vitacura Gardens The SPHERE instrument attached to the VLT Wide-field view of the star-forming region around the Herbig-Haro object HH 46/47
Aerial view of ESO's Headquarters Vitacura Gardens The SPHERE instrument attached to the VLT Wide-field view of the star-forming region around the Herbig-Haro object HH 46/47
The Echelle Spectrograph Comet 1P/Halley
The Echelle Spectrograph Comet 1P/Halley
« Previous 1 | ... | 165 | 166 | 167 | 168 | 169 | 170  
Showing 8789 to 8834 of 8834
Bookmark and Share

Also see our