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Latest Images

Selected background radio continuum sources for...

Selected background radio continuum sources for the SMC (left panel) and the LMC (right ...

Hongxing Chen et al, The Astronomical Journal 169 5

Properties for our selected cold H I structures...

Properties for our selected cold H I structures overplotted on the H I column density ma...

Hongxing Chen et al, The Astronomical Journal 169 5

Gaussian decomposition for Source 1 from the SM...

Gaussian decomposition for Source 1 from the SMC. The top panel shows the H I emission s...

Hongxing Chen et al, The Astronomical Journal 169 5

Cumulative distribution functions (CDF) of fitt...

Cumulative distribution functions (CDF) of fitted Gaussian components for selected SMC a...

Hongxing Chen et al, The Astronomical Journal 169 5

Zoomed-in view of Source 2 in the LMC. Source 2...

Zoomed-in view of Source 2 in the LMC. Source 2 is marked as star in these plots. The to...

Hongxing Chen et al, The Astronomical Journal 169 5

All fitting results of the SMC emission and abs...

All fitting results of the SMC emission and absorption spectra described in Section 4. T...

Hongxing Chen et al, The Astronomical Journal 169 5

CDF of different properties of our selected sou...

CDF of different properties of our selected sources in the LMC and SMC for all lines of ...

Hongxing Chen et al, The Astronomical Journal 169 5

The CNM fraction as a function of the total H I...

The CNM fraction as a function of the total H I column density. We also include data fro...

Hongxing Chen et al, The Astronomical Journal 169 5

All fitting results of the LMC emission and abs...

All fitting results of the LMC emission and absorption spectra described in Section 4. T...

Hongxing Chen et al, The Astronomical Journal 169 5

Figure 9 continued.

Figure 9 continued.

Hongxing Chen et al, The Astronomical Journal 169 5

Left: MCELS Hα image of SGS LMC 1. The OB assoc...

Left: MCELS Hα image of SGS LMC 1. The OB association LH15 is marked in red. The H II re...

Guan-Hong Li et al, The Astronomical Journal 169 5

Left: MCELS Hα image of SGS LMC 1. The 25′ radi...

Left: MCELS Hα image of SGS LMC 1. The 25′ radius circular region is plotted in a red da...

Guan-Hong Li et al, The Astronomical Journal 169 5

MCELS Hα image of SGS LMC 1 superposed with gre...

MCELS Hα image of SGS LMC 1 superposed with green contours of 12CO(1–0) emission observe...

Guan-Hong Li et al, The Astronomical Journal 169 5

Upper panel: the G vs. GBP − GRP CMD of stars o...

Upper panel: the G vs. GBP − GRP CMD of stars overlaid with stellar evolutionary tracks ...

Guan-Hong Li et al, The Astronomical Journal 169 5

Upper panel: the G vs. GBP − GRP CMD of stars o...

Upper panel: the G vs. GBP − GRP CMD of stars overlaid with stellar evolutionary tracks ...

Guan-Hong Li et al, The Astronomical Journal 169 5

Color composite of MCELS Hα image (green) and A...

Color composite of MCELS Hα image (green) and ATCA+Parkes H I column density map (red). ...

Guan-Hong Li et al, The Astronomical Journal 169 5

The 2nd moment map of the ATCA+Parkes H I 21 cm...

The 2nd moment map of the ATCA+Parkes H I 21 cm line data cube from S. Kim et al. (2003).

Guan-Hong Li et al, The Astronomical Journal 169 5

Illustration of our method. Panels (a) is a ske...

Illustration of our method. Panels (a) is a sketch of the richness-mass (N–M) relation m...

Yen-Ting Lin et al, The Astronomical Journal 169 5

Redshift evolution of total stellar mass contai...

Redshift evolution of total stellar mass contained in red member galaxies, for three set...

Yen-Ting Lin et al, The Astronomical Journal 169 5

Illustration of how our method can be used to d...

Illustration of how our method can be used to derive mass–observable relations at differ...

Yen-Ting Lin et al, The Astronomical Journal 169 5

Similar to Figure 4, but for the stellar mass a...

Similar to Figure 4, but for the stellar mass assembly history of BCGs. There appears to...

Yen-Ting Lin et al, The Astronomical Journal 169 5

Similar to Figure 4, but for BCG-to-total stell...

Similar to Figure 4, but for BCG-to-total stellar mass ratio. For a given cluster mass b...

Yen-Ting Lin et al, The Astronomical Journal 169 5

Probability density and cumulative distribution...

Probability density and cumulative distribution of log10(M200m) for...

Yen-Ting Lin et al, The Astronomical Journal 169 5

Probability density of richness for different m...

Probability density of richness for different mass and redshift ranges.

Yen-Ting Lin et al, The Astronomical Journal 169 5

The spectra (gray) and best-fit model (dark blu...

The spectra (gray) and best-fit model (dark blue) with maximal stellar mass of three Bal...

Josephine F. W. Baggen et al, The Astrophysical Journal Letters 977 1

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