activity
20182023
most citedOrbital and spectral characterization of the benchmark T-type brown dwarf HD 19467B

26 citations · 26 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2021

Mapping Luminous Hot Stars in the Galaxy

E. Zari, H. -W. Rix, N. Frankel +4

[Abridged] Luminous hot stars dominate the stellar energy input to the interstellar medium throughout cosmological time, they are laboratories to test theories of stellar evolution…

astro-ph.EP202026 cited

Orbital and spectral characterization of the benchmark T-type brown dwarf HD 19467B

A. -L. Maire, K. Molaverdikhani, S. Desidera +42

Context. Detecting and characterizing substellar companions for which the luminosity, mass, and age can be determined independently is of utter importance to test and calibrate the…

astro-ph.GA2020

The Strength of the Dynamical Spiral Perturbation in the Galactic Disk

Anna-Christina Eilers, David W. Hogg, Hans-Walter Rix +4

The mean Galactocentric radial velocities of luminous red giant stars within the mid-plane of the Milky Way reveal a spiral signature, which could plaus…

astro-ph.GA2020

Keeping it Cool: Much Orbit Migration, yet Little Heating, in the Galactic Disk

Neige Frankel, Jason Sanders, Yuan-Sen Ting +1

A star in the Milky Way's disk can now be at a Galactocentric radius quite distant from its birth radius for two reasons: either its orbit has become eccentric through radial heati…

astro-ph.GA2019

The Inside-out Growth of the Galactic Disk

Neige Frankel, Jason Sanders, Hans-Walter Rix +2

We quantify the inside-out growth of the Milky Way's low-alpha stellar disk, modelling the ages, metallicities and Galactocentric radii of APOGEE red clump stars with 6 < R < 13 kp…

astro-ph.GA2019

Spatial variations in the Milky Way disc metallicity-age relation

Diane K. Feuillet, Neige Frankel, Karin Lind +5

Stellar ages are a crucial component to studying the evolution of the Milky Way. Using Gaia DR2 distance estimates, it is now possible to estimate stellar ages for a larger volume…