Latest Images

Schematic illustration of the outflow model. Th...

Schematic illustration of the outflow model. The arrows indicate the inflow and outflow....

Jun-Rong Liu et al, The Astrophysical Journal Letters 1007 1

Blackbody luminosity versus temperature measure...

Blackbody luminosity versus temperature measured from the red envelope in LRDs (circles)...

Jun-Rong Liu et al, The Astrophysical Journal Letters 1007 1

Observed versus model-predicted FWHMs of the br...

Observed versus model-predicted FWHMs of the broad-line component. Both kinetic and scat...

Jun-Rong Liu et al, The Astrophysical Journal Letters 1007 1

Distribution of Balmer break strengths in LRDs....

Distribution of Balmer break strengths in LRDs. The shaded region shows the expected ran...

Jun-Rong Liu et al, The Astrophysical Journal Letters 1007 1

Distribution of Balmer decrements in LRDs. The ...

Distribution of Balmer decrements in LRDs. The shaded region shows the expected range fr...

Jun-Rong Liu et al, The Astrophysical Journal Letters 1007 1

The spectral energy distribution of TDE2025aarm...

The spectral energy distribution of TDE2025aarm at ≃30–40 days after the optical discove...

Tatsuya Matsumoto and Tsvi Piran, The Astrophysical Journal Letters 1007 1

The possible locations of the SSA peak marked a...

The possible locations of the SSA peak marked as shaded regions, obtained for the CNM de...

Tatsuya Matsumoto and Tsvi Piran, The Astrophysical Journal Letters 1007 1

(Top) The same as Figure 1 but possible synchro...

(Top) The same as Figure 1 but possible synchrotron spectra are presented, which can pro...

Tatsuya Matsumoto and Tsvi Piran, The Astrophysical Journal Letters 1007 1

Multiwavelength light curves of TDE2025aarm. Th...

Multiwavelength light curves of TDE2025aarm. The purple shaded regions represent the pos...

Tatsuya Matsumoto and Tsvi Piran, The Astrophysical Journal Letters 1007 1

Time-series analysis of the events illustrated ...

Time-series analysis of the events illustrated in Figure 1. Panels (a)–(c) show the EUV ...

Daye Lim et al, The Astrophysical Journal Letters 1007 1

Scaling relation between damping time (τ) and o...

Scaling relation between damping time (τ) and oscillation period (P). (a) EUV brightenin...

Daye Lim et al, The Astrophysical Journal Letters 1007 1

Representative examples of analyzed events. (a)...

Representative examples of analyzed events. (a) An EUV brightening observed on 2025 Marc...

Daye Lim et al, The Astrophysical Journal Letters 1007 1

Distributions of QPP quality factors. Probabili...

Distributions of QPP quality factors. Probability density distributions of the quality f...

Daye Lim et al, The Astrophysical Journal Letters 1007 1

Median of the plasma environment and compositio...

Median of the plasma environment and composition parameters under different PVI threshol...

Jiayang Xi et al, The Astrophysical Journal Letters 1007 1

Median value of the alpha-to-proton temperature...

Median value of the alpha-to-proton temperature ratio under different PVI thresholds. Th...

Jiayang Xi et al, The Astrophysical Journal Letters 1007 1

Example of the differential behaviors of alpha ...

Example of the differential behaviors of alpha particles and protons near the coherent s...

Jiayang Xi et al, The Astrophysical Journal Letters 1007 1

Conditional median of the normalized temperatur...

Conditional median of the normalized temperature variations for protons (top row) and al...

Jiayang Xi et al, The Astrophysical Journal Letters 1007 1

Weighted distributions of the final semimajor a...

Weighted distributions of the final semimajor axes and obliquities of HJs formed in our ...

Hareesh Gautham Bhaskar et al, The Astrophysical Journal Letters 1007 1

Final semimajor axes and obliquities of HJs for...

Final semimajor axes and obliquities of HJs formed in our fiducial simulations. Panel (a...

Hareesh Gautham Bhaskar et al, The Astrophysical Journal Letters 1007 1

The observed projected obliquity distribution o...

The observed projected obliquity distribution of hot Jupiters (HJs; with mass >1 MJup) a...

Hareesh Gautham Bhaskar et al, The Astrophysical Journal Letters 1007 1

Marginalized distributions of companion eccentr...

Marginalized distributions of companion eccentricity (panel (a)), HJ obliquity (panel (b...

Hareesh Gautham Bhaskar et al, The Astrophysical Journal Letters 1007 1

Comparison of the analytical expression for the...

Comparison of the analytical expression for the obliquity envelope with secular simulati...

Hareesh Gautham Bhaskar et al, The Astrophysical Journal Letters 1007 1

Projected obliquities and inclinations of HJs f...

Projected obliquities and inclinations of HJs from our simulations. The x-axis shows the...

Hareesh Gautham Bhaskar et al, The Astrophysical Journal Letters 1007 1

Distribution of final obliquities and semimajor...

Distribution of final obliquities and semimajor axes of HJs in our three-planet simulati...

Hareesh Gautham Bhaskar et al, The Astrophysical Journal Letters 1007 1

The final obliquities and semimajor axes of HJs...

The final obliquities and semimajor axes of HJs in our secular simulations. The black do...

Hareesh Gautham Bhaskar et al, The Astrophysical Journal Letters 1007 1

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