¡¡Fotazo!! Gracias mil por la mención. 💜
¡¡Fotazo!! Gracias mil por la mención. 💜
Congratulations to Thomas and the whole team of volunteers!
This way we can define the maximum amount of deformation these pulsars might have. For example the maximum deformation that pulsar J0437−4715 could have is less than 100 microns for a neutron star of radius 10 km!
The Crab Nebula as seen in the X-ray and optical band. The Crab pulsar is in the center of the image.
The LIGO - Virgo - KAGRA (LVK) collaboration recently conducted a new search for extremely faint continuous gravitational waves from isolated neutron stars, specifically 45 known pulsars, using data from the first part of the fourth observing run (O4a). (1/7)
Exactly nine years ago, on the 11th of February 2016, the LIGO - Virgo Collaboration announced the direct observation of gravitational waves to the world (1/4)
Today is International Day of Women and Girls in Science, working every day to make science more…let’s hear it from some of the women of the Virgo Collaboration! 👩🔬
¡Hola Ángel! Ninguna molestia, muchas gracias por tu interés con el podcast y por preguntar. Todo bien. Madre e hija estamos aprendiendo cada día la una de la otra. Una faceta más en mi vida. :)
So true!