Latest Images

The diagnostic band area ratio (BAR) vs. L and ...

The diagnostic band area ratio (BAR) vs. L and H chondrite petrologic type. (a). Plot th...

Pengyue Wang et al, The Astrophysical Journal Letters 985 1

The diagnostic band area ratio (BAR) vs. LL cho...

The diagnostic band area ratio (BAR) vs. LL chondrite petrologic type. BAR increases wit...

Pengyue Wang et al, The Astrophysical Journal Letters 985 1

Abundances of mineral phases in ordinary chondr...

Abundances of mineral phases in ordinary chondrites (T. L. Dunn et al. 2010a).

Pengyue Wang et al, The Astrophysical Journal Letters 985 1

The spectrally derived vs. independently determ...

The spectrally derived vs. independently determined petrologic type of LL chondrites. Th...

Pengyue Wang et al, The Astrophysical Journal Letters 985 1

Ratio of the petrologic type of 28 NEAs.

Ratio of the petrologic type of 28 NEAs.

Pengyue Wang et al, The Astrophysical Journal Letters 985 1

Overview of the eruption on 2024 October 3. Pan...

Overview of the eruption on 2024 October 3. Panel (a): an SDO/HMI LOS magnetogram. The r...

Tao Ding et al, The Astrophysical Journal Letters 985 1

The shearing motion, the flux cancellation, and...

The shearing motion, the flux cancellation, and the emerging dipole in AR 13842 prior to...

Tao Ding et al, The Astrophysical Journal Letters 985 1

Onset and eruption of the flux ropes. Panels (a...

Onset and eruption of the flux ropes. Panels (a1)–(a5): the SDO/AIA EUV data. Panel (a6)...

Tao Ding et al, The Astrophysical Journal Letters 985 1

Temporal evolution of flux ropes (sheared arcad...

Temporal evolution of flux ropes (sheared arcades) revealed by NLFFF extrapolation. Pane...

Tao Ding et al, The Astrophysical Journal Letters 985 1

Historical light curves of BL Lac between 2005 ...

Historical light curves of BL Lac between 2005 and 2024. From top to bottom: γ-ray photo...

Iván Agudo et al, The Astrophysical Journal Letters 985 1

Results of the Swift-XRT monitoring campaign of...

Results of the Swift-XRT monitoring campaign of BL Lac. Fluxes F 0.5−2 keV and F 2−10 ke...

Iván Agudo et al, The Astrophysical Journal Letters 985 1

Flux density F ν (black markers; in units of ...

Flux density F ν (black markers; in units of erg cm−2 s−1 Hz−1) at frequency ν (Hz) an...

Iván Agudo et al, The Astrophysical Journal Letters 985 1

Top panels: best fit to the IXPE, XMM-Newton, a...

Top panels: best fit to the IXPE, XMM-Newton, and NuSTAR data and corresponding residual...

Iván Agudo et al, The Astrophysical Journal Letters 985 1

Optical polarization measurements during the IX...

Optical polarization measurements during the IXPE observation. The top panel shows the b...

Iván Agudo et al, The Astrophysical Journal Letters 985 1

Multiwavelength polarization measurements durin...

Multiwavelength polarization measurements during the IXPE observing campaign reported he...

Iván Agudo et al, The Astrophysical Journal Letters 985 1

Null hypothesis probability of a constant model...

Null hypothesis probability of a constant model of the q (red) and u (blue) Stokes param...

Iván Agudo et al, The Astrophysical Journal Letters 985 1

Short millimeter wavelength and radio polarizat...

Short millimeter wavelength and radio polarization measurements during the IXPE observat...

Iván Agudo et al, The Astrophysical Journal Letters 985 1

Sequence of 43 GHz VLBA images of BL Lac from t...

Sequence of 43 GHz VLBA images of BL Lac from the BEAM-ME program at 0.1 mas angular res...

Iván Agudo et al, The Astrophysical Journal Letters 985 1

Panel (a): best fit of the peak line strength (...

Panel (a): best fit of the peak line strength (in erg cm−2 s−1 Å−1) as a function of acc...

Julia Roman-Duval et al, The Astrophysical Journal 985 1

Panel (a): best fit of the peak line strength (...

Panel (a): best fit of the peak line strength (in erg cm−2 s−1 Å−1) as a function of acc...

Julia Roman-Duval et al, The Astrophysical Journal 985 1

The first and third panels show models and obse...

The first and third panels show models and observed spectra and photometry of two massiv...

Julia Roman-Duval et al, The Astrophysical Journal 985 1

Comparison of the observed (green) and modeled ...

Comparison of the observed (green) and modeled Lyα profiles in RECX-11. The red line cor...

Julia Roman-Duval et al, The Astrophysical Journal 985 1

Relation between accretion rate and Lyα luminos...

Relation between accretion rate and Lyα luminosity in K. France et al. (2017). The blue ...

Julia Roman-Duval et al, The Astrophysical Journal 985 1

P Cygni profiles in the C IV doublet for a pair...

P Cygni profiles in the C IV doublet for a pair of O3.5 dwarfs (left panels) and O4–5 gi...

Julia Roman-Duval et al, The Astrophysical Journal 985 1

Narrow absorption components (NACs) in the N V ...

Narrow absorption components (NACs) in the N V (top panels) and C IV (bottom panels) dou...

Julia Roman-Duval et al, The Astrophysical Journal 985 1

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