COMPANIONS to APOGEE STARS. I. A MILKY WAY-SPANNING CATALOG of STELLAR and SUBSTELLAR COMPANION CANDIDATES and THEIR DIVERSE HOSTS

Nicholas W. Troup, David L. Nidever, Nathan De Lee, Joleen Carlberg, Steven R. Majewski, Martin Fernandez, Kevin Covey, S. Drew Chojnowski, Joshua Pepper, Duy T. Nguyen, Keivan Stassun, Duy Cuong Nguyen, John P. Wisniewski, Scott W. Fleming, Dmitry Bizyaev, Peter M. Frinchaboy, D. A. García-Hernández, Jian Ge, Fred Hearty, Szabolcs MeszarosKaike Pan, Carlos Allende Prieto, Donald P. Schneider, Matthew D. Shetrone, Michael F. Skrutskie, John Wilson, Olga Zamora

Research output: Contribution to journalArticle

32 Scopus citations

Abstract

In its three years of operation, the Sloan Digital Sky Survey Apache Point Observatory Galactic Evolution Experiment (APOGEE-1) observed >14,000 stars with enough epochs over a sufficient temporal baseline for the fitting of Keplerian orbits. We present the custom orbit-fitting pipeline used to create this catalog, which includes novel quality metrics that account for the phase and velocity coverage of a fitted Keplerian orbit. With a typical radial velocity precision of ∼100-200 m s-1, APOGEE can probe systems with small separation companions down to a few Jupiter masses. Here we present initial results from a catalog of 382 of the most compelling stellar and substellar companion candidates detected by APOGEE, which orbit a variety of host stars in diverse Galactic environments. Of these, 376 have no previously known small separation companion. The distribution of companion candidates in this catalog shows evidence for an extremely truncated brown dwarf (BD) desert with a paucity of BD companions only for systems with a < 0.1-0.2 AU, with no indication of a desert at larger orbital separation. We propose a few potential explanations of this result, some which invoke this catalog's many small separation companion candidates found orbiting evolved stars. Furthermore, 16 BD and planet candidates have been identified around metal-poor ([Fe/H] < -0.5) stars in this catalog, which may challenge the core accretion model for companions >10MJup. Finally, we find all types of companions are ubiquitous throughout the Galactic disk with candidate planetary-mass and BD companions to distances of ∼6 and ∼16 kpc, respectively.

Original languageEnglish (US)
Article number85
JournalAstronomical Journal
Volume151
Issue number3
DOIs
StatePublished - Mar 2016

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Troup, N. W., Nidever, D. L., Lee, N. D., Carlberg, J., Majewski, S. R., Fernandez, M., Covey, K., Chojnowski, S. D., Pepper, J., Nguyen, D. T., Stassun, K., Nguyen, D. C., Wisniewski, J. P., Fleming, S. W., Bizyaev, D., Frinchaboy, P. M., García-Hernández, D. A., Ge, J., Hearty, F., ... Zamora, O. (2016). COMPANIONS to APOGEE STARS. I. A MILKY WAY-SPANNING CATALOG of STELLAR and SUBSTELLAR COMPANION CANDIDATES and THEIR DIVERSE HOSTS. Astronomical Journal, 151(3), [85]. https://doi.org/10.3847/0004-6256/151/3/85