587 datasets found

Keywords: Late type stars

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  • High resolution NIR RVs of K2-M4 low-mass stars

    We present the results of a precise near-infrared (NIR) radial velocity (RV) survey of 32 low-mass stars with spectral types K2-M4 using CSHELL at the NASA InfraRed Telescope...
  • Carbon and oxygen abundances in FGK stars

    We present carbon and oxygen abundances for 941 FGK stars -the largest such catalog to date. We find that planet-bearing systems are enriched in these elements. We...
  • Chromospheric activity of Southern stars

    I present chromospheric-activity measurements of ~670 F, G, K, and M main-sequence stars in the Southern Hemisphere, from ~8000 archival high-resolution echelle spectra taken at...
  • Stellar rotation for 71 NGC 6811 members

    We present rotation periods for 71 single dwarf members of the open cluster NGC 6811 determined using photometry from NASA's Kepler mission. The results are the first from The...
  • Rotation periods and membership in M34

    We present the results of a 5 month photometric time-series survey for stellar rotation periods combined with a 4 year radial-velocity survey for membership and binarity in the...
  • Multiple star formation in Taurus-Auriga

    We have conducted a high-resolution imaging study of the Taurus-Auriga star-forming region in order to characterize the primordial outcome of multiple star formation and the...
  • Variability of low-mass stars in SDSS Stripe 82

    We present a catalog of periodic stellar variability in the "Stripe 82" region of the Sloan Digital Sky Survey. After aggregating and re-calibrating catalog-level data from the...
  • Polarized SiO masers of VX Sgr

    We present Submillimeter Array observations of high-frequency SiO masers around the supergiant VX Sgr and the semi-regular variable star W Hya. The J=5-4, v=1^28^SiO and...
  • Spitzer IRAC photometry of M, L, and T dwarfs

    We present the results of a program to acquire photometry for 86 late M, L, and T dwarfs using the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. We examine the...
  • Radio observations of late M, L, and T dwarfs

    I present radio observations of 90 dwarf stars and brown dwarfs of spectral type M5-T8. Three sources exhibit radio activity, in addition to the six objects previously detected...
  • Revision of MK luminosity classes

    The Hipparcos parallaxes of cool giants are utilized in two ways in this paper. First, a plot of reduced parallaxes of stars brighter than 6.5, as a function of spectral type,...
  • X-ray emission at the low-mass end

    We have used all tha available data from the Einstein Observatory Imaging Proportional Counter (IPC), and a critical compilation of catalogued optical data, to measure the...
  • Spectroscopic orbits for late-type stars. II.

    We have determined spectroscopic orbital elements for 13 systems - 10 single-lined binaries and three double-lined binaries. For the three binaries with previously published...
  • The BUD sample. I. L dwarf activity sample

    We present the colors and activity of ultracool (M7-L8) dwarfs from the Tenth Data Release of the Sloan Digital Sky Survey (SDSS). We combine previous samples of SDSS M and L...
  • ROSAT data of Nearby Stars

    We present X-ray data for all entries of the Third Catalogue of Nearby Stars (Gliese and Jahreiss, 1991, Cat. ) that have been detected as X-ray sources in the ROSAT all-sky...
  • HARPS Sco-Cen + SOPHIE YNS and HARPS YNS

    The Scorpius-Centaurus (Sco-Cen) young and nearby massive star-forming region is particularly well suited for extrasolar planet searches with both direct imaging and radial...
  • AD Leo spectral observations

    Stellar flares are energetic events occurring in stellar atmospheres. They have been observed on various stars using photometric light curves and spectra. On some cool stars,...
  • Lithium curves of growth

    The Gaia-ESO Survey (GES) is a large public spectroscopic survey that was carried out using the multi-object FLAMES spectrograph at the VLT. The survey provides accurate radial...
  • Dwarfs, giants and supergiants Equivalent widths

    Stellar population studies in the infrared (IR) wavelength range have two main advantages with respect to the optical regime: they probe different populations, because most of...
  • Masses and luminosities for 342 stars

    We present revised basic astrophysical stellar parameters: the masses, luminosities, ages, and radii for 342 stars from the PennState-Torun Centre for Astronomy Planet Search....
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