Will We See a Starship Test This Week? Barring a further delays, the fifth Starship prototype (SN5) could be ready for a static fire and hop test by the end of this week. The post Will We See a Starship Test This Week? appeared first on Universe Today. Universe Today Go to Source
Revealing the relation between black-hole growth and host-galaxy compactness among star-forming galaxies. (arXiv:2007.04987v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Ni_Q/0/1/0/all/0/1">Q. Ni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brandt_W/0/1/0/all/0/1">W. N. Brandt</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yang_G/0/1/0/all/0/1">G. Yang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Leja_J/0/1/0/all/0/1">J. Leja</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_C/0/1/0/all/0/1">C.-T. J. Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Luo_B/0/1/0/all/0/1">B. Luo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Matharu_J/0/1/0/all/0/1">J. Matharu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sun_M/0/1/0/all/0/1">M. Sun</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vito_F/0/1/0/all/0/1">F. Vito</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Xue_Y/0/1/0/all/0/1">Y. Q. Xue</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_K/0/1/0/all/0/1">K. Zhang</a> Recent studies show that a […]
The Universe at z>10: Predictions for JWST from the UniverseMachine DR1. (arXiv:2007.04988v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Behroozi_P/0/1/0/all/0/1">Peter Behroozi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Conroy_C/0/1/0/all/0/1">Charlie Conroy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wechsler_R/0/1/0/all/0/1">Risa H. Wechsler</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hearin_A/0/1/0/all/0/1">Andrew Hearin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Williams_C/0/1/0/all/0/1">Christina C. Williams</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Moster_B/0/1/0/all/0/1">Benjamin P. Moster</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yung_L/0/1/0/all/0/1">L. Y. Aaron Yung</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Somerville_R/0/1/0/all/0/1">Rachel S. Somerville</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gottlober_S/0/1/0/all/0/1">Stefan Gottlöber</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yepes_G/0/1/0/all/0/1">Gustavo Yepes</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Endsley_R/0/1/0/all/0/1">Ryan Endsley</a> The James Webb […]
Searching for debris discs in the 30 Myr open cluster IC 4665. (arXiv:2007.04992v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Miret_Roig_N/0/1/0/all/0/1">Núria Miret-Roig</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Huelamo_N/0/1/0/all/0/1">Nuria Huélamo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bouy_H/0/1/0/all/0/1">Hervé Bouy</a> Context: Debris discs orbiting young stars are key to understand dust evolution and the planetary formation process. We take advantage of a recent membership analysis of the 30 Myr nearby open cluster […]
Joint analysis of 6dFGS and SDSS peculiar velocities for the growth rate of cosmic structure and tests of gravity. (arXiv:2007.04993v1 [astro-ph.CO]) <a href="http://arxiv.org/find/astro-ph/1/au:+Said_K/0/1/0/all/0/1">Khaled Said</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Colless_M/0/1/0/all/0/1">Matthew Colless</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Magoulas_C/0/1/0/all/0/1">Christina Magoulas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lucey_J/0/1/0/all/0/1">John R. Lucey</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hudson_M/0/1/0/all/0/1">Michael J. Hudson</a> Measurement of peculiar velocities by combining redshifts and distance indicators is a powerful way to measure the […]
Relaxing Cosmological Neutrino Mass Bounds with Unstable Neutrinos. (arXiv:2007.04994v1 [hep-ph]) <a href="http://arxiv.org/find/hep-ph/1/au:+Escudero_M/0/1/0/all/0/1">Miguel Escudero</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Lopez_Pavon_J/0/1/0/all/0/1">Jacobo Lopez-Pavon</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Rius_N/0/1/0/all/0/1">Nuria Rius</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Sandner_S/0/1/0/all/0/1">Stefan Sandner</a> At present, cosmological observations set the most stringent bound on the neutrino mass scale. Within the standard cosmological model ($Lambda$CDM), the Planck collaboration reports $sum m_nu < 0.12,text{eV}$ at 95% CL. This bound, […]
GASP XXX. The spatially resolved SFR-Mass relation in stripping galaxies in the local universe. (arXiv:2007.04996v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Vulcani_B/0/1/0/all/0/1">B. Vulcani</a> (INAF-OaPD), <a href="http://arxiv.org/find/astro-ph/1/au:+Poggianti_B/0/1/0/all/0/1">B. M. Poggianti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tonnesen_S/0/1/0/all/0/1">S. Tonnesen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+McGee_S/0/1/0/all/0/1">S. L. McGee</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Moretti_A/0/1/0/all/0/1">A. Moretti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fritz_J/0/1/0/all/0/1">J. Fritz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gullieuszik_M/0/1/0/all/0/1">M. Gullieuszik</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jaffe_Y/0/1/0/all/0/1">Y. L. Jaffe</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Franchetto_A/0/1/0/all/0/1">A. Franchetto</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tomicic_N/0/1/0/all/0/1">N. Tomicic</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mingozzi_M/0/1/0/all/0/1">M. Mingozzi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bettoni_D/0/1/0/all/0/1">D. […]
Planck intermediate results. LVII. Joint Planck LFI and HFI data processing. (arXiv:2007.04997v1 [astro-ph.CO]) <a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_Planck/0/1/0/all/0/1">Planck Collaboration</a>: <a href="http://arxiv.org/find/astro-ph/1/au:+Akrami_Y/0/1/0/all/0/1">Y. Akrami</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Andersen_K/0/1/0/all/0/1">K. J. Andersen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ashdown_M/0/1/0/all/0/1">M. Ashdown</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Baccigalupi_C/0/1/0/all/0/1">C. Baccigalupi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ballardini_M/0/1/0/all/0/1">M. Ballardini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Banday_A/0/1/0/all/0/1">A. J. Banday</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barreiro_R/0/1/0/all/0/1">R. B. Barreiro</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bartolo_N/0/1/0/all/0/1">N. Bartolo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Basak_S/0/1/0/all/0/1">S. Basak</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Benabed_K/0/1/0/all/0/1">K. Benabed</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bernard_J/0/1/0/all/0/1">J.-P. Bernard</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bersanelli_M/0/1/0/all/0/1">M. Bersanelli</a>, […]
A search for optical and near-infrared counterparts of the compact binary merger GW190814. (arXiv:2007.04998v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Thakur_A/0/1/0/all/0/1">A. L. Thakur</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dichiara_S/0/1/0/all/0/1">S. Dichiara</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Troja_E/0/1/0/all/0/1">E. Troja</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chase_E/0/1/0/all/0/1">E. A. Chase</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sanchez_Ramirez_R/0/1/0/all/0/1">R. Sanchez-Ramirez</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Piro_L/0/1/0/all/0/1">L. Piro</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fryer_C/0/1/0/all/0/1">C. L. Fryer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Butler_N/0/1/0/all/0/1">N. R. Butler</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Watson_A/0/1/0/all/0/1">A. M. Watson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wollaeger_R/0/1/0/all/0/1">R. T. Wollaeger</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ambrosi_E/0/1/0/all/0/1">E. Ambrosi</a>, <a […]
The relation between the diffuse X-ray luminosity and the radio power of the central AGN in galaxy groups. (arXiv:2007.04999v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Pasini_T/0/1/0/all/0/1">T. Pasini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bruggen_M/0/1/0/all/0/1">M. Brūggen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gasperin_F/0/1/0/all/0/1">F. de Gasperin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Birzan_L/0/1/0/all/0/1">L. Bîrzan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+OSullivan_E/0/1/0/all/0/1">E. O'Sullivan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Finoguenov_A/0/1/0/all/0/1">A. Finoguenov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jarvis_M/0/1/0/all/0/1">M. Jarvis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gitti_M/0/1/0/all/0/1">M. Gitti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brighenti_F/0/1/0/all/0/1">F. Brighenti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Whittam_I/0/1/0/all/0/1">I.H. Whittam</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Collier_J/0/1/0/all/0/1">J.D. Collier</a>, <a […]
Core-collapse supernova neutrino emission and detection informed by state-of-the-art three-dimensional numerical models. (arXiv:2007.05000v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Nagakura_H/0/1/0/all/0/1">Hiroki Nagakura</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Burrows_A/0/1/0/all/0/1">Adam Burrows</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vartanyan_D/0/1/0/all/0/1">David Vartanyan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Radice_D/0/1/0/all/0/1">David Radice</a> Based on our recent three-dimensional core-collapse supernova (CCSN) simulations including both exploding and non-exploding models, we study the detailed neutrino signals in representative terrestrial neutrino observatories, Super-Kamiokande (Hyper-Kamiokande), DUNE, […]
Revised and new proper motions for confirmed and candidate Milky Way dwarf galaxies. (arXiv:2007.05011v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+McConnachie_A/0/1/0/all/0/1">Alan W. McConnachie</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Venn_K/0/1/0/all/0/1">Kim A. Venn</a> A new derivation of systemic proper motions of Milky Way satellites is presented, and applied to 59 confirmed or candidate dwarf galaxy satellites using Gaia Data Release 2. This constitutes all known […]
Dense output for highly oscillatory numerical solutions. (arXiv:2007.05013v1 [physics.comp-ph]) <a href="http://arxiv.org/find/physics/1/au:+Agocs_F/0/1/0/all/0/1">F. J. Agocs</a>, <a href="http://arxiv.org/find/physics/1/au:+Hobson_M/0/1/0/all/0/1">M. P. Hobson</a>, <a href="http://arxiv.org/find/physics/1/au:+Handley_W/0/1/0/all/0/1">W. J. Handley</a>, <a href="http://arxiv.org/find/physics/1/au:+Lasenby_A/0/1/0/all/0/1">A. N. Lasenby</a> We present a method to construct a continuous extension (otherwise known as dense output) for a numerical routine in the special case of the numerical solution being a scalar-valued function […]
On the accretion of a new group of galaxies onto Virgo: I. Internal kinematics of nine in-falling dEs. (arXiv:2007.05021v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Bidaran_B/0/1/0/all/0/1">Bahar Bidaran</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pasquali_A/0/1/0/all/0/1">Anna Pasquali</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lisker_T/0/1/0/all/0/1">Thorsten Lisker</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Coccato_L/0/1/0/all/0/1">Lodovico Coccato</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Falcon_Barroso_J/0/1/0/all/0/1">Jesus Falcón-Barroso</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ven_G/0/1/0/all/0/1">Glenn van de Ven</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Peletier_R/0/1/0/all/0/1">Reynier Peletier</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Emsellem_E/0/1/0/all/0/1">Eric Emsellem</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Grebel_E/0/1/0/all/0/1">Eva K. Grebel</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barbera_F/0/1/0/all/0/1">Francesco La Barbera</a>, <a […]
A fast-growing tilt instability of detached circumplanetary disks. (arXiv:2007.05022v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Martin_R/0/1/0/all/0/1">Rebecca G. Martin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_Z/0/1/0/all/0/1">Zhaohuan Zhu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Armitage_P/0/1/0/all/0/1">Philip J. Armitage</a> Accretion disks in binary systems can exhibit a tilt instability, arising from the interaction between components of the tidal potential and dissipation. Using a linear analysis, we show that the aspect ratios and outer […]
CMZoom: Survey Overview and First Data Release. (arXiv:2007.05023v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Battersby_C/0/1/0/all/0/1">Cara Battersby</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Keto_E/0/1/0/all/0/1">Eric Keto</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Walker_D/0/1/0/all/0/1">Daniel Walker</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barnes_A/0/1/0/all/0/1">Ashley Barnes</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Callanan_D/0/1/0/all/0/1">Daniel Callanan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ginsburg_A/0/1/0/all/0/1">Adam Ginsburg</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hatchfield_H/0/1/0/all/0/1">H Perry Hatchfield</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Henshaw_J/0/1/0/all/0/1">Jonathan Henshaw</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kauffmann_J/0/1/0/all/0/1">Jens Kauffmann</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kruijssen_J/0/1/0/all/0/1">J. M. Diederik Kruijssen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Longmore_S/0/1/0/all/0/1">Steven N. Longmore</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lu_X/0/1/0/all/0/1">Xing Lu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mills_E/0/1/0/all/0/1">Elisabeth A. C. Mills</a>, <a […]
Damped Lyman-$alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model. (arXiv:2007.05040v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Gioia_S/0/1/0/all/0/1">Serafina Di Gioia</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cristiani_S/0/1/0/all/0/1">Stefano Cristiani</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lucia_G/0/1/0/all/0/1">Gabriella De Lucia</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Xie_L/0/1/0/all/0/1">Lizhi Xie</a> Using the GAEA semi-analytic model, we analyse the connection between Damped Lyman-$alpha$ systems (DLAs) and HI in galaxies. Our state-of-the-art semi-analytic model is tuned to […]
Goldstone Apple Valley Radio Telescope Observations of 2012 Solar Eclipse: A Multi-wavelength study of cm-wavelength Gyroresonance Emission from Active Regions. (arXiv:2007.05058v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Velusamy_T/0/1/0/all/0/1">T. Velusamy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kuiper_T/0/1/0/all/0/1">T. B. H Kuiper</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dorcey_S/0/1/0/all/0/1">S. M. Levin R. Dorcey</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kreuser_Jenkins_N/0/1/0/all/0/1">N. Kreuser-Jenkins</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Leflang_J/0/1/0/all/0/1">J. Leflang</a> Goldstone Apple Valley Radio Telescope (GAVRT) is a science education partnership among NASA, […]
Parker Solar Probe Gives a Unique Perspective on Comet NEOWISE Comet watchers have enjoying the newly-discovered NEOWISE comet since it was first spotted in March 2020. Now that it’s visible with the naked eye, in dark sky conditions, all kinds of Earthly observers are checking the visitor out. But NASA’s Parker Solar Probe has another […]
Watch the Incredible Plume of Dust from Africa Cross the Entire Atlantic Ocean Dust plumes are a natural phenomena, part of Earth’s nutrient cycle. They occur when high-velocity winds pick up tiny dry particles from the Earth’s surface and carry them long distances. Every summer, dust plumes from Africa’s Sahara desert travel across the Atlantic […]
