output
19932026
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations

Showing 2017 · astro-ph.SRShow all

14 papers · 2 filters

astro-ph.SR2017★ 4 cited

The VLT-FLAMES Tarantula Survey

Jorick S. Vink, C. J. Evans, J. Bestenlehner +5

We present a number of notable results from the VLT-FLAMES Tarantula Survey (VFTS), an ESO Large Program during which we obtained multi-epoch medium-resolution optical spectroscopy…

astro-ph.SR2017★ 70 cited

In-depth study of moderately young but extremely red, very dusty substellar companion HD206893B

P. Delorme, T. Schmidt, M. Bonnefoy +47

The substellar companion HD206893b has recently been discovered by direct imaging of its disc-bearing host star with the SPHERE instrument. We investigate the atypical properties o…

astro-ph.SR2017★ 11 cited

The Association of a J-burst with a Solar Jet

D. E. Morosan, P. T. Gallagher, R. A. Fallows +56

Context. The Sun is an active star that produces large-scale energetic events such as solar flares and coronal mass ejections and numerous smaller-scale events such as solar jets.…

astro-ph.SR2017★ 16 cited

The massive multiple system HD 64315

J. Lorenzo, S. Simon-Diaz, I. Negueruela +4

The O6 Vn star HD 64315 is believed to belong to the star-forming region known as NGC 2467, but previous distance estimates do not support this association. We explore the multiple…

astro-ph.SR2017★ 35 cited

Galactic Bulge Population II Cepheids in the VVV Survey: Period-Luminosity Relations and a Distance to the Galactic Center

A. Bhardwaj, M. Rejkuba, D. Minniti +7

We present the near-infrared observations of population II Cepheids in the Galactic bulge from VVV survey. We identify 340 population II Cepheids in the Galactic bulge from VVV sur…

astro-ph.SR2017★ 60 cited

The low-mass content of the massive young star cluster RCW 38

Koraljka Muzic, Rainer Schoedel, Alexander Scholz +4

RCW 38 is a deeply embedded young (~1 Myr), massive star cluster located at a distance of 1.7 kpc. Twice as dense as the Orion Nebula Cluster, orders of magnitude denser than other…