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Top panel: [Eu/Fe] as a function of [Fe/H] for ...

Top panel: [Eu/Fe] as a function of [Fe/H] for RPE stars with available Th and Dy measur...

Miji Jeong et al, The Astrophysical Journal 1005 1

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Upper panel: abundance ratios ([X/Fe]) of J1222...

Upper panel: abundance ratios ([X/Fe]) of J1222 for heavier elements (Z ≥ 35) as a funct...

Miji Jeong et al, The Astrophysical Journal 1005 1

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Box plot comparison of the elemental abundances...

Box plot comparison of the elemental abundances ([X/Fe]) of the J1222 and 514 non-RPE an...

Miji Jeong et al, The Astrophysical Journal 1005 1

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Observed spectrum (black dots) and synthetic sp...

Observed spectrum (black dots) and synthetic spectra in the CH G band near 4308–4315 Å (...

Miji Jeong et al, The Astrophysical Journal 1005 1

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Chemical-abundance patterns of eight stars: J12...

Chemical-abundance patterns of eight stars: J1222 (red), the actinide-boost candidate CS...

Miji Jeong et al, The Astrophysical Journal 1005 1

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Top panel: determination of the carbon isotope ...

Top panel: determination of the carbon isotope ratio (12C/13C) for J1222. The black squa...

Miji Jeong et al, The Astrophysical Journal 1005 1

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SYN results derived for J1222 for important neu...

SYN results derived for J1222 for important neutron-capture elements, from left to right...

Miji Jeong et al, The Astrophysical Journal 1005 1

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Normalized, order-combined spectrum of J1222, c...

Normalized, order-combined spectrum of J1222, covering the wavelength range 3600–10000 Å.

Miji Jeong et al, The Astrophysical Journal 1005 1

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Top: after correcting the spectral index for ex...

Top: after correcting the spectral index for extinction, many of the older Class I YSOs ...

Michael Connelley et al, The Astrophysical Journal 1005 1

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Top: the close correlation between magnitudes o...

Top: the close correlation between magnitudes of visual extinction and spectral index, s...

Michael Connelley et al, The Astrophysical Journal 1005 1

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Along with a broad trend toward lower spectral ...

Along with a broad trend toward lower spectral index with increasing gravity (age), ther...

Michael Connelley et al, The Astrophysical Journal 1005 1

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The mass accretion rate is shown vs. the log(g)...

The mass accretion rate is shown vs. the log(g) of the central star (top panel) and vs. ...

Michael Connelley et al, The Astrophysical Journal 1005 1

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The Brγ line flux, corrected for extinction and...

The Brγ line flux, corrected for extinction and distance, overall declines as stars evol...

Michael Connelley et al, The Astrophysical Journal 1005 1

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Here we compare veiling and the Brγ line, as we...

Here we compare veiling and the Brγ line, as we use both as accretion tracers. The veili...

Michael Connelley et al, The Astrophysical Journal 1005 1

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On this plot of mass vs. age, the dotted vector...

On this plot of mass vs. age, the dotted vectors show how much the mass of each YSO shou...

Michael Connelley et al, The Astrophysical Journal 1005 1

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We see a wide range of extinction values for ag...

We see a wide range of extinction values for ages under ∼5 Myr (log(g) < 4.0) with no ap...

Michael Connelley et al, The Astrophysical Journal 1005 1

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PD, PA, count rate, and hardness ratio (top to ...

PD, PA, count rate, and hardness ratio (top to bottom) for HS 2022 (blue), IMS 2022 (yel...

Romana Mikušincová et al, The Astrophysical Journal 1005 1

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Normalized Stokes parameters U/I versus Q/I for...

Normalized Stokes parameters U/I versus Q/I for the IXPE observations of Cyg X-3. HS 202...

Romana Mikušincová et al, The Astrophysical Journal 1005 1

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Dependence of the PD (top), PA (middle), and co...

Dependence of the PD (top), PA (middle), and count rate (bottom) on the orbital phase. E...

Romana Mikušincová et al, The Astrophysical Journal 1005 1

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Dependence of PD (top) and PA (bottom) on energ...

Dependence of PD (top) and PA (bottom) on energy in the 2–8 keV band. HS 2022 in blue sq...

Romana Mikušincová et al, The Astrophysical Journal 1005 1

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IXPE PDs (data points, HS 2022 in blue and HS 2...

IXPE PDs (data points, HS 2022 in blue and HS 2023 in green) with two PD models fitted t...

Romana Mikušincová et al, The Astrophysical Journal 1005 1

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Top to bottom: unfolded EFE (energy flux) spect...

Top to bottom: unfolded EFE (energy flux) spectra of Stokes I, Q, and U, comparing the s...

Romana Mikušincová et al, The Astrophysical Journal 1005 1

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X-ray versus radio flux density diagram. Blue, ...

X-ray versus radio flux density diagram. Blue, orange, green, and red asterisks indicate...

Romana Mikušincová et al, The Astrophysical Journal 1005 1

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Peak r-band absolute magnitude vs. redshift, wi...

Peak r-band absolute magnitude vs. redshift, with projected histograms. The magnitude er...

Daichi Hiramatsu et al, The Astrophysical Journal 1005 1

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Left: GP light curves in absolute magnitude in ...

Left: GP light curves in absolute magnitude in each filter (g, c, G, r, o, and i from to...

Daichi Hiramatsu et al, The Astrophysical Journal 1005 1

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