Latest Images

Example of subtracted image. The two bottom fig...

A Method for Optimal Image Subtraction

Example of subtracted image. The two bottom figures of the panel are the original images...

Alard & Lupton, The Astrophysical Journal 503 1 325

Noise in the subtracted image. The image on the...

A Method for Optimal Image Subtraction

Noise in the subtracted image. The image on the left is the subtracted image normalized ...

Alard & Lupton, The Astrophysical Journal 503 1 325

Examples of bright giant light curves. The x‐ax...

A Method for Optimal Image Subtraction

Examples of bright giant light curves. The x‐axes are days, the y‐axes are percentage va...

Alard & Lupton, The Astrophysical Journal 503 1 325

Periodic variables. The x‐axes represent the ph...

A Method for Optimal Image Subtraction

Periodic variables. The x‐axes represent the phase, the y‐axes are percentage variation ...

Alard & Lupton, The Astrophysical Journal 503 1 325

Comparison of our temperatures with those from ...

The Temperature Structure of 30 Nearby ...

Comparison of our temperatures with those from Einstein MPC, EXOSAT, and Ginga (David et...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Cluster temperature maps. Contours show ROSAT P...

The Temperature Structure of 30 Nearby ...

Cluster temperature maps. Contours show ROSAT PSPC brightness; gray scale shows ASCA tem...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Cluster temperature maps. Contours show ROSAT P...

The Temperature Structure of 30 Nearby ...

Cluster temperature maps. Contours show ROSAT PSPC brightness; gray scale shows ASCA tem...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Cluster temperature maps. Contours show ROSAT P...

The Temperature Structure of 30 Nearby ...

Cluster temperature maps. Contours show ROSAT PSPC brightness; gray scale shows ASCA tem...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Temperature and specific entropy maps of A3395 ...

The Temperature Structure of 30 Nearby ...

Temperature and specific entropy maps of A3395 (see text). Left panels are similar to Fi...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Radial projected temperature profiles. Crosses ...

The Temperature Structure of 30 Nearby ...

Radial projected temperature profiles. Crosses are centered on the emission‐weighted rad...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Radial projected temperature profiles. Crosses ...

The Temperature Structure of 30 Nearby ...

Radial projected temperature profiles. Crosses are centered on the emission‐weighted rad...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Radial projected temperature profiles. Crosses ...

The Temperature Structure of 30 Nearby ...

Radial projected temperature profiles. Crosses are centered on the emission‐weighted rad...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Normalized temperature profiles of 19 relativel...

The Temperature Structure of 30 Nearby ...

Normalized temperature profiles of 19 relatively symmetric clusters, plotted against rad...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Normalized temperature profiles of several clus...

The Temperature Structure of 30 Nearby ...

Normalized temperature profiles of several cluster subsets. Error bars are omitted for c...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Normalized profiles of symmetric clusters (thos...

The Temperature Structure of 30 Nearby ...

Normalized profiles of symmetric clusters (those shown in Fig. 5, without AWM 7 and A216...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Temperature profiles from cluster simulations o...

The Temperature Structure of 30 Nearby ...

Temperature profiles from cluster simulations overlaid on our results. Light‐shaded band...

Temperature Structure of Clusters, The Astrophysical Journal 503 1 77

Neutrino production distribution inside the hom...

Neutrinos and Supermassive Stars: Prosp...

Neutrino production distribution inside the homologous core (unnormalized): the distribu...

Shi & Fuller, The Astrophysical Journal 503 1 307

Time evolution of the neutrino luminosity accor...

Neutrinos and Supermassive Stars: Prosp...

Time evolution of the neutrino luminosity according to eq. (17), for ...

Shi & Fuller, The Astrophysical Journal 503 1 307

Solid lines: Spectra of ...

Neutrinos and Supermassive Stars: Prosp...

Solid lines: Spectra of ﹩\nu _{e}\,\overline{\nu }_{e}﹩ (upper) and ...

Shi & Fuller, The Astrophysical Journal 503 1 307

Event rates from the supermassive star neutrino...

Neutrinos and Supermassive Stars: Prosp...

Event rates from the supermassive star neutrino background in several new‐generation det...

Shi & Fuller, The Astrophysical Journal 503 1 307

ASCA (a) SIS and (b) GIS spectra of NGC 4579. T...

Detection of an Iron K Emission Line fr...

ASCA (a) SIS and (b) GIS spectra of NGC 4579. The best‐fit model consists of an R‐S ther...

Terashima et al., The Astrophysical Journal 503 1 212

ASCA (a) SIS and (b) GIS spectra of NGC 4579. T...

Detection of an Iron K Emission Line fr...

ASCA (a) SIS and (b) GIS spectra of NGC 4579. The best‐fit model consists of an R‐S ther...

Terashima et al., The Astrophysical Journal 503 1 212

Data/model ratio for the best‐fit continuum mod...

Detection of an Iron K Emission Line fr...

Data/model ratio for the best‐fit continuum model around an iron K emission line. The cr...

Terashima et al., The Astrophysical Journal 503 1 212

Confidence contours for the line energy and int...

Detection of an Iron K Emission Line fr...

Confidence contours for the line energy and intensity. The energy scale is redshift corr...

Terashima et al., The Astrophysical Journal 503 1 212

Confidence contours for the line width (Gaussia...

Detection of an Iron K Emission Line fr...

Confidence contours for the line width (Gaussian σ) and intensity. The contours correspo...

Terashima et al., The Astrophysical Journal 503 1 212

Geometry of the blob–magnetic field interaction...

A New Instability of Accretion Disks ar...

Geometry of the blob–magnetic field interaction. The two panels correspond to different ...

Vietri & Stella, The Astrophysical Journal 503 1 350

Geometry of the reference systems of § 2.1. The...

A New Instability of Accretion Disks ar...

Geometry of the reference systems of § 2.1. The K frame is inertial; its z axis is along...

Vietri & Stella, The Astrophysical Journal 503 1 350

Time dependence of the rate of Joule heating in...

Joule Heating and the Thermal Evolution...

Time dependence of the rate of Joule heating integrated over the star volume and normali...

Miralles, Urpin, & Konenkov, The Astrophysical Journal 503 1 368

Thermal evolution of the FP model with and with...

Joule Heating and the Thermal Evolution...

Thermal evolution of the FP model with and without Joule heating. Curve 1: Be = 1.5 × 10...

Miralles, Urpin, & Konenkov, The Astrophysical Journal 503 1 368

Thermal evolution of the PS model with and with...

Joule Heating and the Thermal Evolution...

Thermal evolution of the PS model with and without Joule heating. Curve 1: Be = 1.5 × 10...

Miralles, Urpin, & Konenkov, The Astrophysical Journal 503 1 368

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