Latest Images

X‐ray color‐color diagram of 4U 1702−429. Each ...

Observation of Kilohertz Quasi‐periodic...

X‐ray color‐color diagram of 4U 1702−429. Each point represents a 256 s average over the...

Markwardt, Strohmayer, & Swank, The Astrophysical Journal Letters 512 2 L125

Average 2–25 keV PCA power spectrum for observa...

Observation of Kilohertz Quasi‐periodic...

Average 2–25 keV PCA power spectrum for observations on July 30, after shifting the cent...

Markwardt, Strohmayer, & Swank, The Astrophysical Journal Letters 512 2 L125

Broadband power spectrum of 4U 1702−429 startin...

Observation of Kilohertz Quasi‐periodic...

Broadband power spectrum of 4U 1702−429 starting on July 26.6 (bottom curve) and July 30...

Markwardt, Strohmayer, & Swank, The Astrophysical Journal Letters 512 2 L125

Dynamic power spectrum showing ≈330 Hz pulsatio...

Observation of Kilohertz Quasi‐periodic...

Dynamic power spectrum showing ≈330 Hz pulsations during a burst from 4U 1702−429. The c...

Markwardt, Strohmayer, & Swank, The Astrophysical Journal Letters 512 2 L125

The 6 cm radio image of Sco X‐1 on 1997.638 at ...

High‐Resolution Parallax Measurements o...

The 6 cm radio image of Sco X‐1 on 1997.638 at 02:15 UT: contour levels are −0.3, 0.3, 0...

Bradshaw, Fomalont, & Geldzahler, The Astrophysical Journal Letters 512 2 L121

As in Fig. 1, but for 1998.162 at 13:05 UT. Con...

High‐Resolution Parallax Measurements o...

As in Fig. 1, but for 1998.162 at 13:05 UT. Contour levels are −0.2, 0.2, 0.4, 0.6, 0.8,...

Bradshaw, Fomalont, & Geldzahler, The Astrophysical Journal Letters 512 2 L121

Sco X‐1 6 cm east‐west (top) and north‐south (b...

High‐Resolution Parallax Measurements o...

Sco X‐1 6 cm east‐west (top) and north‐south (bottom) residual positions after removing ...

Bradshaw, Fomalont, & Geldzahler, The Astrophysical Journal Letters 512 2 L121

Plots of extinction vs. declination for cut 1 a...

Measuring Galactic Extinction: A Test

Plots of extinction vs. declination for cut 1 and cut 2 of AG. The first cut is centered...

Arce & Goodman, The Astrophysical Journal Letters 512 2 L135

A plot of the 100 μm dust emission vs. declinat...

Measuring Galactic Extinction: A Test

A plot of the 100 μm dust emission vs. declination for a part of cut 1. The light line i...

Arce & Goodman, The Astrophysical Journal Letters 512 2 L135

Peculiar velocities as a function of angle from...

A Large‐scale Bulk Flow of Galaxy Clusters

Peculiar velocities as a function of angle from the apex of the bulk flow. Symbol sizes ...

Hudson et al., The Astrophysical Journal Letters 512 2 L79

Peculiar velocities projected onto a plane betw...

A Large‐scale Bulk Flow of Galaxy Clusters

Peculiar velocities projected onto a plane between ﹩\mathrm{SGX}\,=0﹩ and ...

Hudson et al., The Astrophysical Journal Letters 512 2 L79

Peculiar velocities and bulk flow directions in...

A Large‐scale Bulk Flow of Galaxy Clusters

Peculiar velocities and bulk flow directions in Galactic coordinates (Aitoff projection)...

Hudson et al., The Astrophysical Journal Letters 512 2 L79

Co‐added infrared images of Cygnus A: F110W ima...

An Edge‐brightened Bicone in the Nuclea...

Co‐added infrared images of Cygnus A: F110W image (1.1 μm) (top left); F160W image (1.6 ...

Tadhunter et al., The Astrophysical Journal Letters 512 2 L91

Schematic diagram showing a possible model for ...

An Edge‐brightened Bicone in the Nuclea...

Schematic diagram showing a possible model for the edge‐brightened bicone structure in C...

Tadhunter et al., The Astrophysical Journal Letters 512 2 L91

High‐state (epoch 2, solid line) and low‐state ...

On the Absence of Broad Mg II Emission ...

High‐state (epoch 2, solid line) and low‐state (epoch 5, dotted line) continuum‐subtract...

Goad et al., The Astrophysical Journal Letters 512 2 L95

Comparison between the normalized 1996 HST/FOS ...

On the Absence of Broad Mg II Emission ...

Comparison between the normalized 1996 HST/FOS Mg II emission line profile (smoothed to ...

Goad et al., The Astrophysical Journal Letters 512 2 L95

(a) Comparison between the C IV (solid line) an...

On the Absence of Broad Mg II Emission ...

(a) Comparison between the C IV (solid line) and Mg II (dashed line) emission line profi...

Goad et al., The Astrophysical Journal Letters 512 2 L95

Constraint on the redshift of assembly for the ...

Consequences of Feedback from Early Sup...

Constraint on the redshift of assembly for the Milky Way disk obtained from early SN fee...

Natarajan, The Astrophysical Journal Letters 512 2 L105

Top panel: orbital energy relative to the satel...

Tidal Streams as Probes of the Galactic...

Top panel: orbital energy relative to the satellite's ﹩\Delta E﹩ for all particles unbou...

Johnston et al., The Astrophysical Journal Letters 512 2 L109

Left‐hand panels: maximum number of captured pa...

Tidal Streams as Probes of the Galactic...

Left‐hand panels: maximum number of captured particles for fixed ﹩v_{\mathrm{circ}\,}﹩ a...

Johnston et al., The Astrophysical Journal Letters 512 2 L109

Bootstrapped errors in the potential calculated...

Tidal Streams as Probes of the Galactic...

Bootstrapped errors in the potential calculated with N stars. The filled triangles, squa...

Johnston et al., The Astrophysical Journal Letters 512 2 L109

Cumulative area of the source plane A>, at ...

Deep Counts of Submillimeter Galaxies

Cumulative area of the source plane A>, at ﹩z_{s}=2﹩, that experiences a magnification g...

Blain et al., The Astrophysical Journal Letters 512 2 L87

Systematic differences in the inferred counts f...

Deep Counts of Submillimeter Galaxies

Systematic differences in the inferred counts for the 80% Smail et al. (1998) sample (so...

Blain et al., The Astrophysical Journal Letters 512 2 L87

Cumulative sub‐mm counts corrected for lens mag...

Deep Counts of Submillimeter Galaxies

Cumulative sub‐mm counts corrected for lens magnification as listed in Table 1. The resu...

Blain et al., The Astrophysical Journal Letters 512 2 L87

A representation of the CO observations made wi...

Molecular Gas Depletion and Starbursts ...

A representation of the CO observations made with the NRAO 12 m telescope (the 55...

Gao & Solomon, The Astrophysical Journal Letters 512 2 L99

(a) CO luminosity vs. ﹩S_{\mathrm{sep}\,}﹩ for ...

Molecular Gas Depletion and Starbursts ...

(a) CO luminosity vs. ﹩S_{\mathrm{sep}\,}﹩ for 50 LIG mergers. A strong correlation hold...

Gao & Solomon, The Astrophysical Journal Letters 512 2 L99

(a) Cataloged SGR 1806−20 bursts from 1983 Octo...

SGR 1806−20 Is a Set of Independent Rel...

(a) Cataloged SGR 1806−20 bursts from 1983 October to November (103 bursts). Burst size ...

Palmer, The Astrophysical Journal Letters 512 2 L113

(a) Cumulative burst fluence for interval B (33...

SGR 1806−20 Is a Set of Independent Rel...

(a) Cumulative burst fluence for interval B (33 bursts). Each vertical line is a burst. ...

Palmer, The Astrophysical Journal Letters 512 2 L113

(a) Cumulative burst fluence for interval A, ex...

SGR 1806−20 Is a Set of Independent Rel...

(a) Cumulative burst fluence for interval A, exclusive of the burst at DOY 297.940 (dash...

Palmer, The Astrophysical Journal Letters 512 2 L113

Spectra of HCN, H13CN, and HC15N; for coordinat...

The Detection of Extragalactic 15N: Con...

Spectra of HCN, H13CN, and HC15N; for coordinates, see Chin et al. (1997) and Henkel, Wh...

Chin et al., The Astrophysical Journal Letters 512 2 L143

SEARCH TERM(S)

PUBLICATIONS

  • 25423
  • 316557
  • 16491
  • 48804

YEAR RANGE:

1995
2014

CONTENT TYPE

AUTHOR