Skip to content
  • Rationale
  • Invited Speakers
  • Program
  • Supermassive Black Hole Logo Supermassive Black Hole Logo Supermassive Black Hole Logo
  • Talks & Posters
    • Accretion on small scales
    • Binary Systems / Gravitational Waves
    • Cosmic Growth
    • Local Universe
    • Poster
  • Alphabetical Order
  • Rationale
  • Invited Speakers
  • Program
  • Supermassive Black Hole Logo Supermassive Black Hole Logo Supermassive Black Hole Logo
  • Talks & Posters
    • Accretion on small scales
    • Binary Systems / Gravitational Waves
    • Cosmic Growth
    • Local Universe
    • Poster
  • Alphabetical Order
  • Rationale
  • Invited Speakers
  • Program
  • Supermassive Black Hole Logo Supermassive Black Hole Logo Supermassive Black Hole Logo
  • Talks & Posters
    • Accretion on small scales
    • Binary Systems / Gravitational Waves
    • Cosmic Growth
    • Local Universe
    • Poster
  • Alphabetical Order
Talks & Postersadministrador2020-12-05T20:03:21+01:00
  • All
  • Accretion on small scales
  • Binary Systems / Gravitational Waves
  • Cosmic Growth
  • Local Universe
  • Poster
Pamela Henriquez2020-12-06T15:33:51+01:00

Pulsar timing array limits on supermassive BH binaries within 500 Mpc – Maria Charisi

Pamela Henriquez2020-12-06T15:12:40+01:00

Stellar winds pump the heart of the Milky Way – Diego Calderón

Pamela Henriquez2020-12-06T15:57:26+01:00

Hypervelocity Red Clump Stars in the Galactic Bulge – Alonso Luna

Pamela Henriquez2020-12-06T15:57:11+01:00

Optical properties of highly accreting quasars – Alenka Negrete

Pamela Henriquez2020-12-06T15:08:44+01:00

Host galaxies properties of 47 Type 1 AGN in MaNGA – Edgar Cortes Suárez

Pamela Henriquez2020-12-06T15:06:58+01:00

The first measurement of the quasar lifetime distribution – Ilya Khrykin

Pamela Henriquez2020-12-06T15:05:53+01:00

Semi-analytic modeling of AGNs: auto-correlation function and halo occupation – Taira Oogi

Pamela Henriquez2020-12-06T15:02:27+01:00

AGN powered by IMBHs: scaling relations and (often) rapid growth – Igor Chilingarian

Pamela Henriquez2020-12-06T15:01:17+01:00

Consistent predictions for IMBHs,Chandra observations of probable IMBHs in the Virgo cluster – Alister Graham

Pamela Henriquez2020-12-06T14:56:06+01:00

Formation of SMBH seeds in nuclear star clusters via gas accretion and runaway collisions -Arpan Das

Pamela Henriquez2020-12-06T14:53:58+01:00

Black hole growth on parsec scales revealed by interferometry – Konrad Tristram

Pamela Henriquez2020-12-06T14:52:33+01:00

The most massive SMBHs at early epoch of the Universe – Fuyan Bian

Previous123456789Next
© 2020 Universidad de Concepción.
X
Go to Top