Astronomy Image Explorer

Latest Images

First row, right panel: unsharp-masked WFPC2/F5...

First row, right panel: unsharp-masked WFPC2/F555W image of the double nucleus in NGC 44...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

Image Details View Article

Trajectories of the BH that is kicked from the ...

Trajectories of the BH that is kicked from the center of NGC 4486B. The different-colore...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

Image Details View Article

Expected GW recoil kick magnitude, Vkick, as a ...

Expected GW recoil kick magnitude, Vkick, as a function of the premerger BH mass ratio, ...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

Image Details View Article

Top: radial profile of the retrograde orbit fra...

Top: radial profile of the retrograde orbit fraction from the best-fit Schwarzschild mod...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

Image Details View Article

The top panel presents the projected luminosity...

The top panel presents the projected luminosity density of NGC 4486B (black dots) derive...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

Image Details View Article

Trajectory of the BH that is placed at the cent...

Trajectory of the BH that is placed at the center of NGC 4486B without any recoil kick. ...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

Image Details View Article

Time evolution of the galaxy and the SMBH binar...

Time evolution of the galaxy and the SMBH binary parameters. Top left: volume–density pr...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

Image Details View Article

Best-fit Schwarzschild models with (top) and wi...

Best-fit Schwarzschild models with (top) and without (bottom) retrograde orbits, each an...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

Image Details View Article

Examples of a metric type II radio burst event ...

Examples of a metric type II radio burst event on 2015 November 4. The spectrum was chos...

X.-N. Wang et al, The Astrophysical Journal 1001 1

Image Details View Article

The CME and its driven shock from the SOHO LASC...

The CME and its driven shock from the SOHO LASCO/C2 instruments on 2000 December 18. The...

X.-N. Wang et al, The Astrophysical Journal 1001 1

Image Details View Article

Postage stamps of the edge-on galaxy UVCANDELS ...

Postage stamps of the edge-on galaxy UVCANDELS 20524 show that while the F160W image is ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

UVCANDELS 08062 has a bright off-center feature...

UVCANDELS 08062 has a bright off-center feature most clearly seen in F275W and F435W, wi...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

Postage stamps for the face-on spiral UVCANDELS...

Postage stamps for the face-on spiral UVCANDELS 25207 show in F435W a bright bulge and c...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

log SFR and log stellar mass of the eight galax...

log SFR and log stellar mass of the eight galaxies in our sample as calculated with the ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

Eight galaxies of the “Gold Sample” are shown i...

Eight galaxies of the “Gold Sample” are shown in the F435W band. These galaxies have a v...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

Shown are postage stamps and property maps of 1...

Shown are postage stamps and property maps of 10335 in pixel coordinates. Top: HST F275W...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

Evolution of the log ΣSFR–log ...

Evolution of the log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩correlation over the past ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

The two panels show how the slope, normalizatio...

The two panels show how the slope, normalization, and redshift vary between each galaxy’...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩co...

log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩correlation fit lines for all galaxies are ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

The two panels show how the slope, normalizatio...

The two panels show how the slope, normalization, and scatter of each galaxy’s regional ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

UVCANDELS 05386 is cataloged as a pair, with th...

UVCANDELS 05386 is cataloged as a pair, with the dimmer object to the right likely a com...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

Projected radial sSFR profiles for UVCANDELS ID...

Projected radial sSFR profiles for UVCANDELS IDs 08218, 22456, and 23475 all show a net ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

The projected radial profiles of galaxy 25207 h...

The projected radial profiles of galaxy 25207 have similar shapes across all properties....

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

Shown is UVCANDELS 08218. Clear star-forming cl...

Shown is UVCANDELS 08218. Clear star-forming clumps appear in F275W and remain visible i...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

Evolving log ΣSFR–log ...

Evolving log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩correlations for UVCANDELS IDs 053...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

Image Details View Article

ANNOUNCEMENTS

Take the AstroExplorer for a spin!

Be sure to try the search and sorting features, which were added based on user feedback; browse and find the links to videos and interactive figures in our Journal articles; find AAS Research Notes; or notice that new publishers have begun adding their figures to the AIE. Get in touch to hear more!