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Initial parameters for evolved massive binaries...

Initial parameters for evolved massive binaries at 15 (left) and 30 Myr (right). Each in...

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Comparison between the number of evolved massiv...

Comparison between the number of evolved massive binaries resulting from fiducial models...

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Comparison between the number of evolved massiv...

Comparison between the number of evolved massive binaries resulting from fiducial models...

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Predicted mass distribution for binaries compri...

Predicted mass distribution for binaries comprising an OB star paired with an HeS, NS, o...

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Same as Figure 4, but the results are obtained ...

Same as Figure 4, but the results are obtained with the idealized mass transfer assumption.

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Same as Figure 4, but the results are based on ...

Same as Figure 4, but the results are based on an alternative SN explosion assumption as...

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Same as Figure 2 but for an age of 30 Myr.

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Same as Figure 2 but for an age of 80 Myr.

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Same as Figure 2 but for an age of 50 Myr.

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Predicted properties of OB-type MS star binarie...

Predicted properties of OB-type MS star binaries containing a helium-burning star (reddi...

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Distribution of our models in the CMD at 15 Myr...

Distribution of our models in the CMD at 15 Myr, matching the estimated age of NGC 2100....

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Panel (a): predicted numbers of postinteraction...

Panel (a): predicted numbers of postinteraction binaries as a function of age in a coeva...

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Predicted properties of OB+BH binaries as a fun...

Predicted properties of OB+BH binaries as a function of cluster age. The color coding re...

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Similar to Figure 1 but for ages of 10, 30, 60,...

Similar to Figure 1 but for ages of 10, 30, 60, and 100 Myr.

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Same as Figure 3, but the sample size is reduce...

Same as Figure 3, but the sample size is reduced to 60%, 40%, 20%, and 10% in each panel.

Chen Wang et al, The Astrophysical Journal Letters 975 1

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Environment of Hedgehog. We show the distributi...

Environment of Hedgehog. We show the distribution of neighboring galaxies from Karachent...

Jiaxuan Li et al, The Astrophysical Journal Letters 975 1

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The SBF measurements for Hedgehog using the IMA...

The SBF measurements for Hedgehog using the IMACS i-band data (top panels) and the Legac...

Jiaxuan Li et al, The Astrophysical Journal Letters 975 1

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The V-band absolute magnitude and size of Hedge...

The V-band absolute magnitude and size of Hedgehog, together with other isolated quiesce...

Jiaxuan Li et al, The Astrophysical Journal Letters 975 1

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Cutout images of Hedgehog from the Legacy Surve...

Cutout images of Hedgehog from the Legacy Surveys DR10 (left), the deep and high-resolut...

Jiaxuan Li et al, The Astrophysical Journal Letters 975 1

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ArtPop models of Hedgehog...

ArtPop models of Hedgehog at different distances. We generate thes...

Jiaxuan Li et al, The Astrophysical Journal Letters 975 1

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Light plains are smooth, flat deposits with sha...

Light plains are smooth, flat deposits with sharp contacts and a higher reflectance than...

Barbara Giuri et al, The Planetary Science Journal 5 10

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Light plains deposits filled in pink on an equi...

Light plains deposits filled in pink on an equirectangular projection of the Moon center...

Barbara Giuri et al, The Planetary Science Journal 5 10

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Different views of the distribution of LPs on t...

Different views of the distribution of LPs on the lunar globe (orthographic projection)....

Barbara Giuri et al, The Planetary Science Journal 5 10

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(a) Smooth deposits showing flow-like features ...

(a) Smooth deposits showing flow-like features in the Inghirami crater region (68.7°W 47...

Barbara Giuri et al, The Planetary Science Journal 5 10

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Imbrium Sculpture region (a) FeO map after P. G...

Imbrium Sculpture region (a) FeO map after P. G. Lucey et al. (2000) (b) LP deposits as ...

Barbara Giuri et al, The Planetary Science Journal 5 10

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