Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Vega, Justin"'
While astronomers often assume that exoplanets are perfect spheres when analyzing observations, the subset of these distant worlds that are subject to strong tidal forces and/or rapid rotations are expected to be distinctly ellipsoidal or even triaxi
Externí odkaz:
http://arxiv.org/abs/2409.00167
Autor:
Roelofs, Freek, Blackburn, Lindy, Lindahl, Greg, Doeleman, Sheperd S., Johnson, Michael D., Arras, Philipp, Chatterjee, Koushik, Emami, Razieh, Fromm, Christian, Fuentes, Antonio, Knollmueller, Jakob, Kosogorov, Nikita, Mueller, Hendrik, Patel, Nimesh, Raymond, Alexander, Tiede, Paul, Traianou, Thalia, Vega, Justin
The next-generation Event Horizon Telescope (ngEHT) will be a significant enhancement of the Event Horizon Telescope (EHT) array, with $\sim 10$ new antennas and instrumental upgrades of existing antennas. The increased $uv$-coverage, sensitivity, an
Externí odkaz:
http://arxiv.org/abs/2212.11355
Autor:
Chatterjee, Koushik, Chael, Andrew, Tiede, Paul, Mizuno, Yosuke, Emami, Razieh, Fromm, Christian, Ricarte, Angelo, Blackburn, Lindy, Roelofs, Freek, Johnson, Michael D., Doeleman, Sheperd S., Arras, Philipp, Fuentes, Antonio, Knollmüller, Jakob, Kosogorov, Nikita, Lindahl, Greg, Müller, Hendrik, Patel, Nimesh, Raymond, Alexander, Traianou, Efthalia, Vega, Justin
In the past few years, the Event Horizon Telescope (EHT) has provided the first-ever event horizon-scale images of the supermassive black holes (BHs) (M87*) and Sagittarius A$^*$ (Sgr A*). The next-generation EHT project is an extension of the EHT ar
Externí odkaz:
http://arxiv.org/abs/2212.01804
Autor:
Long, Feng, Andrews, Sean M., Vega, Justin, Wilner, David J., Chandler, Claire J., Ragusa, Enrico, Teague, Richard, Pérez, Laura M., Calvet, Nuria, Carpenter, John M., Henning, Thomas, Kwon, Woojin, Linz, Hendrik, Ricci, Luca
We present high resolution millimeter continuum and CO line observations for the circumbinary disk around V892 Tau to constrain the stellar and disk properties. The total mass of the two near-equal-mass A stars is estimated to be $6.0\pm0.2\,M_{\odot
Externí odkaz:
http://arxiv.org/abs/2105.02918
Autor:
Roelofs, Freek, Blackburn, Lindy, Lindahl, Greg, Doeleman, Sheperd S., Johnson, Michael D., Arras, Philipp, Chatterjee, Koushik, Emami, Razieh, Fromm, Christian, Fuentes, Antonio, Knollmüller, Jakob, Kosogorov, Nikita, Müller, Hendrik, Patel, Nimesh, Raymond, Alexander, Tiede, Paul, Traianou, Efthalia, Vega, Justin
Publikováno v:
Galaxies (2075-4434); Feb2023, Vol. 11 Issue 1, p12, 30p
