Search Publications

The Multiplicity of M Dwarfs in Young Moving Groups
DOI: 10.3847/1538-4357/aa859d Bibcode: 2017ApJ...846...93S

Yee, Jennifer C.; Montet, Benjamin T.; Bowler, Brendan P. +12 more

We image 104 newly identified low-mass (mostly M-dwarf) pre-main sequence (PMS) members of nearby young moving groups (YMGs) with Magellan Adaptive Optics (MagAO) and identify 27 stellar binaries with instantaneous projected separation as small as 40 mas. Fifteen were previously unknown. The total number of multiple systems in this sample includin…

2017 The Astrophysical Journal
Gaia 17
The AB Doradus system revisited: The dynamical mass of AB Dor A/C
DOI: 10.1051/0004-6361/201730641 Bibcode: 2017A&A...607A..10A

Ros, E.; Lestrade, J. -F.; Tognelli, E. +6 more

Context. The study of pre-main-sequence (PMS) stars with model-independent measurements of their masses is essential to check the validity of theoretical models of stellar evolution. The well-known PMS binary AB Dor A/C is an important benchmark for this task, since it displays intense and compact radio emission, which makes possible the applicati…

2017 Astronomy and Astrophysics
Hipparcos 16
Bidirectional reflectance and VIS-NIR spectroscopy of cometary analogues under simulated space conditions
DOI: 10.1016/j.pss.2017.07.009 Bibcode: 2017P&SS..145...14J

Thomas, Nicolas; Fornasier, Sonia; Pommerol, Antoine +7 more

This work is intended to be the second publication in a series of papers reporting on the spectro-photometric properties of cometary analogues measured in the laboratory. Herein, we provide in-situ hyperspectral imaging data in the 0.40-2.35 µm range from three sublimation experiments under simulated space conditions in thermal vacuum from s…

2017 Planetary and Space Science
Rosetta 16
Meet the family - the catalog of known hot subdwarf stars
DOI: 10.1515/astro-2017-0432 Bibcode: 2017OAst...26..164G

Gänsicke, Boris T.; Telting, John H.; Østensen, Roy H. +6 more

In preparation for the upcoming all-sky data releases of the Gaia mission, we compiled a catalog of known hot subdwarf stars and candidates drawn from the literature and yet unpublished databases. The catalog contains 5613 unique sources and provides multi-band photometry from the ultraviolet to the far infrared, ground based proper motions, class…

2017 Open Astronomy
Gaia 16
Discovery of a soft X-ray 8 mHz QPO from the accreting millisecond pulsar IGR J00291+5934
DOI: 10.1093/mnras/stw3344 Bibcode: 2017MNRAS.466.3450F

Sanna, A.; Ferrigno, C.; Papitto, A. +7 more

We report on the analysis of the peculiar X-ray variability displayed by the accreting millisecond X-ray pulsar IGR J00291+5934 in a 80 ks-long joint NuSTAR and XMM-Newton observation performed during the source outburst in 2015. The light curve of the source is characterized by a flaring-like behaviour, with typical rise and decay time-scales of …

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 16
Data processing pipeline for Herschel HIFI
DOI: 10.1051/0004-6361/201731385 Bibcode: 2017A&A...608A..49S

Shipman, R. F.; Sanchez, E.; Braine, J. +26 more

Context. The HIFI instrument on the Herschel Space Observatory performed over 9100 astronomical observations, almost 900 of which were calibration observations in the course of the nearly four-year Herschel mission. The data from each observation had to be converted from raw telemetry into calibrated products and were included in the Herschel Scie…

2017 Astronomy and Astrophysics
Herschel 16
Intrinsic scatter of caustic masses and hydrostatic bias: An observational study
DOI: 10.1051/0004-6361/201730920 Bibcode: 2017A&A...606A..25A

Andreon, S.; Moretti, A.; Wang, J. +1 more

All estimates of cluster mass have some intrinsic scatter and perhaps some bias with true mass even in the absence of measurement errors for example caused by cluster triaxiality and large scale structure. Knowledge of the bias and scatter values is fundamental for both cluster cosmology and astrophysics. In this paper we show that the intrinsic s…

2017 Astronomy and Astrophysics
XMM-Newton 16
Study of the accretion torque during the 2014 outburst of the X-ray pulsar GRO J1744-28
DOI: 10.1093/mnras/stx635 Bibcode: 2017MNRAS.469....2S

Sanna, A.; Esposito, P.; Segreto, A. +9 more

We present the spectral and timing analysis of the X-ray pulsar GRO J1744-28 during its 2014 outburst using data collected with the X-ray satellites Swift, INTEGRAL, Chandra, and XMM-Newton. We derived, by phase-connected timing analysis of the observed pulses, an updated set of the source ephemeris. We were also able to investigate the spin-up of…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 16
A Redshift Survey of the Nearby Galaxy Cluster Abell 2199: Comparison of the Spatial and Kinematic Distributions of Galaxies with the Intracluster Medium
DOI: 10.3847/1538-4357/aa72dc Bibcode: 2017ApJ...842...88S

Hwang, Ho Seong; Park, Changbom; Song, Hyunmi +1 more

We present the results from an extensive spectroscopic survey of the central region of the nearby galaxy cluster Abell 2199 (A2199) at z = 0.03. By combining 775 new redshifts from the MMT/Hectospec observations with the data in the literature, we construct a large sample of 1624 galaxies with measured redshifts at R< 30\prime , whic…

2017 The Astrophysical Journal
Suzaku 16
Stellar dynamics in the strong-lensing central galaxy of Abell 1201: a low stellar mass-to-light ratio, a large central compact mass and a standard dark matter halo
DOI: 10.1093/mnras/stx1573 Bibcode: 2017MNRAS.471..383S

Edge, Alastair C.; Lucey, John R.; Smith, Russell J.

We analyse the stellar kinematics of the z = 0.169 brightest cluster galaxy in Abell 1201, using integral field observations acquired with the Multi-Unit Spectroscopic Explorer on the Very Large Telescope. This galaxy has a gravitationally lensed arc located at unusually small radius (∼5 kpc), allowing us to constrain the mass distribution using l…

2017 Monthly Notices of the Royal Astronomical Society
eHST 16