Telescopes

HI4PI survey map (Image courtesy Benjamin Winkel, Max Planck Institute, and the HI4PI collaboration.)

An article published in the journal “Astronomy & Astrophysics” describes the creation of a map of neutral atomic hydrogen in the Milky Way. An international team of scientists put together data collected by two of the largest steerable radio telescopes in the world, the 100-m Max-Planck radio telescope in Effelsberg, Germany and the 64-m CSIRO radio telescope in Parkes, Australia.

The central part of the Milky Way (Image ESO/VVV Survey/D. Minniti)

An article published in “The Astrophysical Journal Letters” describes the discovery of the relics of an ancient globular cluster in the Milky Way’s central area. A team of astronomers led by Dante Minniti (Universidad AndrĂ©s Bello, Santiago, Chile) and Rodrigo Contreras Ramos (Instituto Milenio de AstrofĂ­sica, Santiago, Chile) used observations from the “Variables in the Via Lactea with VISTA” (VVV) survey carried out with ESO’s VISTA telescope to discover the ancient stars of type RR Lyrae for the first time in that area.

2014 UZ224 orbit (Image JPL Horizons / Sky and Telescope)

David Gerdes, a professor of astrophysics at the University of Michigan, and a number of colleagues associated with the DES (Dark Energy Survey) survey have discovered a new dwarf planet that currently has a distance of about 14 billion kilometers (about 8.5 billion miles) from the Sun. Called for now just 2014 UZ224, it’s among the most distant celestial bodies discovered in the solar system after the dwarf planet Eris and the possible dwarf planet known as V774104 whose discovery was announced in December 2015.

The IRS 43 system (Image courtesy Christian Brinch/NBI/KU)

An article published in “Astrophysical Journal Letters” describes a research on the IRS 43 system, which turned out to be really extraordinary because it’s formed by two very young stars each surrounded by a disk of gas but they share a third much bigger disk. A team of scientists from the Niels Bohr Institute, University of Copenhagen, used the ALMA radio telescope to discover this structure never seen before.

Sequence of interactions between V Hydrae and its companion that cause the ejection of plasma blobs (Image NASA, ESA, and A. Feild (STScI))

An article published in “The Astrophysical Journal” describes a research on the huge plasma blobs ejected by the red giant star V Hydrae. A team of astronomers led by Raghvendra Sahai of NASA’s JPL used the Hubble Space Telescope to study this phenomenon and concluded that the plasma blobs come from another star, a companion of V Hydrae that we can’t see.