Left Muse He Ii And Alma C I1 0 Line Spectra Of The Host Galaxies

Left: MUSE He ii and ALMA [C i](1-0) line spectra of the host galaxies ...
Left: MUSE He ii and ALMA [C i](1-0) line spectra of the host galaxies ...
Mean line profiles of Hα, four He I lines and an He II line at the ...
Mean line profiles of Hα, four He I lines and an He II line at the ...
Left: Continuum-subtracted images of LAB1 and LAB2 in the He II line ...
Left: Continuum-subtracted images of LAB1 and LAB2 in the He II line ...
continued: Here, we show the He ii and [C i] spectra alongside the ...
continued: Here, we show the He ii and [C i] spectra alongside the ...
The H I spectra (left) and their CoGs (right) of three galaxies with ...
The H I spectra (left) and their CoGs (right) of three galaxies with ...
Figure 1 from The emission line sequence of H II galaxies | Semantic ...
Figure 1 from The emission line sequence of H II galaxies | Semantic ...
Large-scale [ ] C II line emission maps derived from the new ALMA ...
Large-scale [ ] C II line emission maps derived from the new ALMA ...
-The left panels show the VLBI spectra of megamasers in UGC 6093 and ...
-The left panels show the VLBI spectra of megamasers in UGC 6093 and ...
Space-resolved spectra and lineouts along the highest intensity of He a ...
Space-resolved spectra and lineouts along the highest intensity of He a ...
Line ratios for He II, C IV, and Lyα for the entire source (black star ...
Line ratios for He II, C IV, and Lyα for the entire source (black star ...
ALMA spectra of [C ii] and underlying continuum of the quasars in our ...
ALMA spectra of [C ii] and underlying continuum of the quasars in our ...
-A comparison between the morphology of He ii emission and V-band ...
-A comparison between the morphology of He ii emission and V-band ...
Spectra of the [C ii] λ157.74 µm emission line for all the new ALMA ...
Spectra of the [C ii] λ157.74 µm emission line for all the new ALMA ...
The probability distribution of DM host for disc and non-disc galaxies ...
The probability distribution of DM host for disc and non-disc galaxies ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...
Spectroscopic line confirmations of the galaxies targeted in this ...
Spectroscopic line confirmations of the galaxies targeted in this ...
Same as Fig. 3 but zooming in on the He ii λ4686 Å line (upper panels ...
Same as Fig. 3 but zooming in on the He ii λ4686 Å line (upper panels ...
The MUSE Hα and ALMA CO(2-1) datacubes reveal similar morphologies at ...
The MUSE Hα and ALMA CO(2-1) datacubes reveal similar morphologies at ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...
HST (left) and MUSE (right) field images of the region around 244-440 ...
HST (left) and MUSE (right) field images of the region around 244-440 ...
Spatial distribution of ALMA and MIRI clumps. From left to right, ALMA ...
Spatial distribution of ALMA and MIRI clumps. From left to right, ALMA ...
Figure A.1 from The VLT-MUSE and ALMA view of the MACS 1931.8-2635 ...
Figure A.1 from The VLT-MUSE and ALMA view of the MACS 1931.8-2635 ...
| Spatially-integrated spectra of the [C II] emission line in the ...
| Spatially-integrated spectra of the [C II] emission line in the ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - IV. No tight ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - IV. No tight ...
Overlay of ALMA CO(2-1) emission (red) on MUSE Hα emission (green) and ...
Overlay of ALMA CO(2-1) emission (red) on MUSE Hα emission (green) and ...
Montage of He I, He II, and C III images and emissivities during a ...
Montage of He I, He II, and C III images and emissivities during a ...
He II emitters at cosmic noon and beyond - Characterising the He II ...
He II emitters at cosmic noon and beyond - Characterising the He II ...
Can we identify the host galaxies of LISA sources? | astrobites
Can we identify the host galaxies of LISA sources? | astrobites
The NGC 1087 galaxy as seen with MUSE on ESO’s VLT and ALMA | ESO Svizzera
The NGC 1087 galaxy as seen with MUSE on ESO’s VLT and ALMA | ESO Svizzera
The Optical Properties of Host Galaxies of Radio Sources in the Coma ...
The Optical Properties of Host Galaxies of Radio Sources in the Coma ...
Researchers detect the host galaxies of quasars in the early universe ...
Researchers detect the host galaxies of quasars in the early universe ...
Integrated central MUSE aperture spectra within a diameter of 3 for HE ...
Integrated central MUSE aperture spectra within a diameter of 3 for HE ...
The NGC 1087 galaxy as seen with MUSE on ESO’s VLT and ALMA | ESO España
The NGC 1087 galaxy as seen with MUSE on ESO’s VLT and ALMA | ESO España
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...
Physics of ULIRGs with MUSE and ALMA: The PUMA project - I. Properties ...

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