Search Publications

Chemical compositions and kinematics of the Hercules stream
DOI: 10.1093/mnras/stw852 Bibcode: 2016MNRAS.460.1356R

Lambert, David L.; Reddy, Bacham E.; Ramya, P. +1 more

An abundance analysis is reported of 58-K giants identified by Famaey et al. (2005, A&A, 430, 165) as highly probable members of the Hercules stream selected from stars north of the celestial equator in the Hipparcos catalogue. The giants have compositions spanning the interval [Fe/H] from -0.17 to +0.42 with a mean value of +0.15 and relative…

2016 Monthly Notices of the Royal Astronomical Society
Hipparcos 13
Long-term R and V-band monitoring of some suitable targets for the link between ICRF and the future Gaia celestial reference frame
DOI: 10.1051/0004-6361/201526676 Bibcode: 2016A&A...587A.112T

Souchay, J.; Taris, F.; Andrei, A. +3 more

Context. The Gaia astrometric mission of the European Space Agency was launched on December 2013. It will provide a catalog of 500 000 quasars. Some of these targets will be chosen to build an optical reference system that will be linked to the International Celestial Reference Frame (ICRF). The astrometric coordinates of these sources will have r…

2016 Astronomy and Astrophysics
Gaia 13
Electric sail option for cometary rendezvous
DOI: 10.1016/j.actaastro.2016.06.020 Bibcode: 2016AcAau.127..684Q

Janhunen, Pekka; Quarta, Alessandro A.; Mengali, Giovanni

The recent successes of the European Rosetta mission have shown the possibility of a close observation with one of the most evasive celestial bodies in the Solar System, the comets, and the practical feasibility of a comet rendezvous to obtain detailed information and in situ measurements. This paper discusses a preliminary study of the transfer t…

2016 Acta Astronautica
Rosetta 13
InSight coordinates determination from direct-to-Earth radio-tracking and Mars topography model
DOI: 10.1016/j.pss.2015.11.003 Bibcode: 2016P&SS..121....1L

Le Maistre, Sébastien

The InSight mission is planned to land on the surface of Mars in September 2016. Close to the equator in Elysium Planitia, in the vicinity of the Curiosity location, the exact landing site coordinates cannot be provided by the navigation team. The direct-to-Earth (DTE) Doppler measurements are rarely included in the early lander localization proce…

2016 Planetary and Space Science
MEx 13
Protoplanetary Disk Shadowing by Gas Infalling onto the Young Star AK Sco
DOI: 10.3847/2041-8205/818/1/L17 Bibcode: 2016ApJ...818L..17G

France, Kevin; Gómez de Castro, Ana I.; Loyd, Robert O. P. +2 more

Young solar-type stars grow through the accretion of material from the circumstellar disk during pre-main-sequence (PMS) evolution. The ultraviolet radiation generated in this process plays a key role in the chemistry and evolution of young planetary disks. In particular, the hydrogen Lyα line (Lyα) etches the disk surface by driving photoevaporat…

2016 The Astrophysical Journal
eHST 13
A VLA Survey for Faint Compact Radio Sources in the Orion Nebula Cluster
DOI: 10.3847/0004-637X/831/2/155 Bibcode: 2016ApJ...831..155S

Williams, Jonathan P.; Sheehan, Patrick D.; Eisner, Josh A. +1 more

We present Karl G. Jansky Very Large Array 1.3, 3.6, and 6 cm continuum maps of compact radio sources in the Orion Nebular Cluster (ONC). We mosaicked 34 arcmin2 at 1.3 cm, 70 arcmin2 at 3.6 cm and 109 arcmin2 at 6 cm, containing 778 near-infrared detected young stellar objects and 190 Hubble Space Telescope-identi…

2016 The Astrophysical Journal
eHST 13
A Symmetric Inner Cavity in the HD 141569A Circumstellar Disk
DOI: 10.3847/0004-637X/818/2/150 Bibcode: 2016ApJ...818..150M

Augereau, J. -C.; Boccaletti, A.; Lagrange, A. -M. +6 more

Some circumstellar disks, called transitional or hybrid disks, present characteristics of both protoplanetary disks (significant amount of gas) and debris disks (evolved structures around young main-sequence stars, composed of second generation dust, from collisions between planetesimals). Therefore, they are ideal astrophysical laboratories to wi…

2016 The Astrophysical Journal
eHST 13
Suzaku Wide-band All-sky Monitor measurements of duration distributions of gamma-ray bursts
DOI: 10.1093/pasj/psw009 Bibcode: 2016PASJ...68S..30O

Yamaoka, Kazutaka; Fukazawa, Yasushi; Hanabata, Yoshitaka +25 more

We report on the T90 and T50 duration distributions and their relations with spectral hardness using 1464 gamma-ray bursts (GRBs), which were observed by the Suzaku Wide-band All-sky Monitor (WAM) from 2005 August 4 to 2010 December 29. The duration distribution is clearly bimodal in three energy ranges (50-120, 120-250, and …

2016 Publications of the Astronomical Society of Japan
INTEGRAL Suzaku 13
Long-term nadir observations of the O2 dayglow by SPICAM IR
DOI: 10.1016/j.pss.2015.12.006 Bibcode: 2016P&SS..122....1G

Montmessin, F.; Fedorova, A.; Korablev, O. +4 more

The O2(a1Δg) dayglow at the 1.27 µm band on Mars is produced by the solar UV photolysis of ozone and quenched in collisions with CO2. The SPICAM IR instrument onboard the Mars Express orbiter observes the O2(a1Δg) emission in the Martian atmosphere starting from 200…

2016 Planetary and Space Science
MEx 13
Kinematics and Magnetic Properties of a Light Bridge in a Decaying Sunspot
DOI: 10.1007/s11207-016-0944-8 Bibcode: 2016SoPh..291.1939F

Guglielmino, S. L.; Romano, P.; Borrero, J. M. +7 more

We present the results obtained by analysing high spatial and spectral resolution data of the solar photosphere acquired by the CRisp Imaging SpectroPolarimeter at the Swedish Solar Telescope on 6 August 2011 of a large sunspot with a light bridge (LB) observed in NOAA AR 11263. These data are complemented by simultaneous Hinode Spectropolarimeter…

2016 Solar Physics
Hinode 13