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Sample and spectral fitting methodology. Left p...

Sample and spectral fitting methodology. Left panel: distribution of the full sample in ...

Liang Wu et al, The Astrophysical Journal Letters 1001 1

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Kinematically consistent decomposition of [O II...

Kinematically consistent decomposition of [O II] and [Ne V] emission lines for the full ...

Liang Wu et al, The Astrophysical Journal Letters 1001 1

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[O II] and [Ne V] line profiles and flux ratios...

[O II] and [Ne V] line profiles and flux ratios as a function of bolometric luminosity. ...

Liang Wu et al, The Astrophysical Journal Letters 1001 1

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SFRs as a function of quasar bolometric luminos...

SFRs as a function of quasar bolometric luminosity. SFRs derived from host [O II] lumino...

Liang Wu et al, The Astrophysical Journal Letters 1001 1

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Magnetic field evolution of the hyperactive mag...

Magnetic field evolution of the hyperactive magnetar. Four snapshots are shown at times ...

Ashley Bransgrove et al, The Astrophysical Journal Letters 1001 1

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Snapshot of ambipolar diffusion at t = 200 yr. ...

Snapshot of ambipolar diffusion at t = 200 yr. (a) Relative velocity between plasma and ...

Ashley Bransgrove et al, The Astrophysical Journal Letters 1001 1

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Thermal evolution of the hyperactive magnetar. ...

Thermal evolution of the hyperactive magnetar. At early times, the temperature drops rap...

Ashley Bransgrove et al, The Astrophysical Journal Letters 1001 1

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Structure of the magnetospheric flare. The colo...

Structure of the magnetospheric flare. The color shows Bϕ/r⊥, and the white curve is the...

Ashley Bransgrove et al, The Astrophysical Journal Letters 1001 1

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Top: continuum-subtracted JWST/MIRI spectra of ...

Top: continuum-subtracted JWST/MIRI spectra of 3I in the ν2 band of H2O from both epochs...

Matthew Belyakov et al, The Astrophysical Journal Letters 1001 1

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Left: a compilation of H2O, CO2, and CH4 produc...

Left: a compilation of H2O, CO2, and CH4 production rates for 3I published in M. R. Comb...

Matthew Belyakov et al, The Astrophysical Journal Letters 1001 1

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Top: coma maps of H2O, CO2, and CH4, computed a...

Top: coma maps of H2O, CO2, and CH4, computed as the molecular column density from a pix...

Matthew Belyakov et al, The Astrophysical Journal Letters 1001 1

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Top: the JWST/NIRSpec PRISM spectrum of 3I in t...

Top: the JWST/NIRSpec PRISM spectrum of 3I in the vicinity of the CH4 ν3 fluorescence ba...

Matthew Belyakov et al, The Astrophysical Journal Letters 1001 1

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Azimuthal profiles of H2O (blue) and CO2 (orang...

Azimuthal profiles of H2O (blue) and CO2 (orange) at ...

Matthew Belyakov et al, The Astrophysical Journal Letters 1001 1

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An example of the continuum modeling procedure ...

An example of the continuum modeling procedure applied to prepare the extracted JWST/MIR...

Matthew Belyakov et al, The Astrophysical Journal Letters 1001 1

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Top: median-stacked images derived from the ful...

Top: median-stacked images derived from the fully calibrated Channel 2 data cubes for th...

Matthew Belyakov et al, The Astrophysical Journal Letters 1001 1

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Normalized number fractions for stars with diff...

Normalized number fractions for stars with different inclinations. The black solid lines...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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A dynamo simulation on the latitudinal distribu...

A dynamo simulation on the latitudinal distribution of the magnetic flux emergence for d...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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Same as Figure 3, but for three temperature bin...

Same as Figure 3, but for three temperature bins of fast rotators. The sample includes p...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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Same as Figure 3, but we allow sini to exceed 1...

Same as Figure 3, but we allow sini to exceed 1 by directly integrating p(sini∣D). This ...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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Same as Figure 4, but for the rotation period. ...

Same as Figure 4, but for the rotation period. We convert Ro to rotation period by using...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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Relations on the proxy of light-curve modulatio...

Relations on the proxy of light-curve modulation Sph. The top left panel shows its relat...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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Top panel: same as Figure 1, but for the flare ...

Top panel: same as Figure 1, but for the flare catalog of B. Seli et al. (2025). Middle ...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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Inclination sini vs. the flaring activity in di...

Inclination sini vs. the flaring activity in different Ro bins. The size of the filled c...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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Rossby number vs. the mean latitude of active r...

Rossby number vs. the mean latitude of active regions. Each black point represents the b...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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Same as Figure 3, but for several larger Ro bin...

Same as Figure 3, but for several larger Ro bins. The bottom right panel shows the relat...

Huiqin Yang et al, The Astrophysical Journal Supplement Series 283 2

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