Rezultati pretraživanja
  1. New semester, new Fellows’ Seminars . Today with Prof and Thomas Tauris who takes us through his magical research into and compact objects.

  2. Scaling K2. I. Revised Parameters for 222,088 K2 Stars and a K2 Planet Radius Valley at 1.9 _{\oplus}$. (arXiv:2001.11511v1 [])

  3. Characterizing hydrostatic mass bias with Mock-X. (arXiv:2001.11508v1 [])

  4. The MASSIVE Survey XIV -- Stellar Velocity Profiles and Kinematic Misalignments from 200 pc to 20 kpc in Massive Early-type Galaxies. (arXiv:2001.11046v1 [])

  5. prije 18 sati
  6. _{\rm{dust}}-M_{\star}$ Relation Hints at the Origin of Particle Traps in Protoplanetary Disks. (arXiv:2001.11045v1 [astro-ph.EP])

  7. 2. velj

    Testing low-redshift cosmic acceleration with large-scale structure. (arXiv:2001.11044v1 [])

  8. 2. velj

    Systematic Variations of CO J=2-1/1-0 Ratio in The Barred Spiral Galaxy M83. (arXiv:2001.11043v1 [])

  9. 1. velj

    Quantifying the Toroidal Flux of Preexisting Flux Ropes of Coronal Mass Ejections

  10. 1. velj

    Probing the Origin of Diffuse Radio Emission in the Cool Core of the Phoenix Galaxy Cluster via

  11. 1. velj

    Hot Subdwarf Stars Identified in Gaia DR2 with Spectra of LAMOST DR6 and DR7. I. Single-lined Spectra

  12. 1. velj

    Toward the Detection of Relativistic Image Doubling in Imaging Atmospheric Cherenkov Telescopes via

  13. 1. velj

    Molecular Oxygen in the Nearest QSO Mrk 231

  14. 1. velj

    Beyond Optical Depth: Future Determination of Ionization History from the Cosmic Microwave Background via

  15. 31. sij
  16. 31. sij

    Constraining dark matter annihilation with HSC low surface brightness galaxies

  17. TFW you're gujju but also an astrophysicist. If you know, you know

  18. 30. sij

    A Neutral Beam Model for High-energy Neutrino Emission from the Blazar TXS 0506+056 via

  19. 30. sij

    Clusters of Galaxies Masquerading as X-Ray Quasars via

Čini se da učitavanje traje već neko vrijeme.

Twitter je možda preopterećen ili ima kratkotrajnih poteškoća u radu. Pokušajte ponovno ili potražite dodatne informacije u odjeljku Status Twittera.