output
20022026
most citedSpectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation

1.4k citations

Showing 2019 · astro-ph.GAShow all

8 papers · 2 filters

astro-ph.GA2019★ 60 cited

LLAMA: The - Relation of the most luminous local AGNs

Turgay Caglar, Leonard Burtscher, Bernhard Brand +17

The - relation is considered a result of co-evolution between the host galaxies and their super-massive black holes. For elliptical-bulge hosting inactive gala…

astro-ph.GA2019★ 75 cited

Metallicity and -element Abundance Gradients along the Sagittarius Stream as Seen by APOGEE

Christian R. Hayes, Steven R. Majewski, Sten Hasselquist +27

Using 3D positions and kinematics of stars relative to the Sagittarius (Sgr) orbital plane and angular momentum, we identify 166 Sgr stream members observed by the Apache Point Obs…

astro-ph.GA2019★ 4 cited

Sardinia Radio Telescope observations of Local Group dwarf galaxies -- I. The cases of NGC6822, IC1613, and WLM

A. Tarchi, P. Castangia, G. Surcis +10

Almost all dwarf galaxies in the Local Group that are not satellites of the Milky Way or M31, belong to either one of two highly-symmetric planes. It is still a matter of debate, w…

astro-ph.GA2019★ 33 cited

A Search for Intrinsic HI 21 cm and OH 18 cm Absorption Toward Compact Radio Sources

Kathryn Grasha, Jeremy Darling, Alberto Bolatto +2

We present the results of a large search for intrinsic HI 21 cm and OH 18 cm absorption in 145 compact radio sources in the redshift range 0.02< z <3.8 with the Green Bank Telescop…

astro-ph.GA2019★ 2 cited

Revisiting the Temperature of the Diffuse ISM with CHESS Sounding Rocket Observations

Nicholas Kruczek, Kevin France, Keri Hoadley +2

Measuring the temperature and abundance patterns of clouds in the interstellar medium (ISM) provides an observational basis for models of the physical conditions within the clouds,…

astro-ph.GA2019★ 10 cited

Ambipolar diffusion in large Prandtl number turbulence

Axel Brandenburg

We study the effects of ambipolar diffusion (AD) on hydromagnetic turbulence. In most of the cases, we use the single fluid approximation where the drift velocity between charged a…