Search Publications

The SSDC contribution to the improvement of knowledge by means of 3D data projections of minor bodies
DOI: 10.1016/j.asr.2018.04.023 Bibcode: 2018AdSpR..62.2306Z

Longobardo, Andrea; Palomba, Ernesto; Zinzi, Angelo +6 more

The latest developments of planetary exploration missions devoted to minor bodies required new solutions to correctly visualize and analyze data acquired over irregularly shaped bodies.

ASI Space Science Data Center (SSDC - ASI, formerly ASDC - ASI Science Data Center) worked on this task since early 2013, when started developing the web tool…

2018 Advances in Space Research
Rosetta 6
Exploring the substellar population in the Hyades open cluster
DOI: 10.1051/0004-6361/201833672 Bibcode: 2018A&A...620A.130P

Rebolo, R.; Lodieu, N.; Pérez-Garrido, A. +1 more


Aims: Our aim is to identify substellar members of the nearby Hyades open star cluster to determine the photometric and spectroscopic properties of brown dwarfs at moderately old ages and extend our knowledge of the substellar mass function of the cluster.
Methods: We cross-matched the 2MASS and WISE public catalogues and measured proper…

2018 Astronomy and Astrophysics
Gaia 6
Far-infrared photometry of OJ 287 with the Herschel Space Observatory
DOI: 10.1051/0004-6361/201732142 Bibcode: 2018A&A...610A..74K

Lähteenmäki, Anne; Tornikoski, Merja; Tammi, Joni +6 more

Context. The blazar OJ 287 has shown a ≈12 year quasi-periodicity over more than a century, in addition to the common properties of violent variability in all frequency ranges. It is the strongest known candidate to have a binary singularity in its central engine. Aim. We aim to better understand the different emission components by searching for …

2018 Astronomy and Astrophysics
Herschel 6
AGB Candidates in the Field of γ Cas1
DOI: 10.48550/arXiv.1805.09191 Bibcode: 2018RMxAA..54..341N

Enke, H.; Nesci, R.; Tuvikene, T. +4 more

We report the spectroscopic and photometric monitoring of a sample of 530 candidate AGB stars in a 5×5 degrees field, selected from the IPHAS catalog; historic light curves were derived from Asiago IR plates taken in the years 1965-1984. We found 10 Miras, 5 stars with long term trends, 3 semiregular and 3 irregular. Spectral types from CCD slit s…

2018 Revista Mexicana de Astronomia y Astrofisica
Gaia 6
High-velocity hot CO emission close to Sgr A*. Herschel/HIFI submillimeter spectral survey toward Sgr A*
DOI: 10.1051/0004-6361/201833684 Bibcode: 2018A&A...616L...1G

Teyssier, D.; Cernicharo, J.; Gerin, M. +3 more

The properties of molecular gas, the fuel that forms stars, inside the cavity of the circumnuclear disk (CND) are not well constrained. We present results of a velocity-resolved submillimeter scan ( 480-1250 GHz) and [C II] 158 µm line observations carried out with Herschel/HIFI toward Sgr A*; these results are complemented by a 2…

2018 Astronomy and Astrophysics
Herschel 6
HATS-59b,c: A Transiting Hot Jupiter and a Cold Massive Giant Planet around a Sun-like Star
DOI: 10.3847/1538-3881/aade54 Bibcode: 2018AJ....156..216S

Arriagada, P.; Butler, R. P.; Crane, J. D. +27 more

We report the first discovery of a multi-planetary system by the HATSouth network, HATS-59b,c, a planetary system with an inner transiting hot Jupiter and an outer cold massive giant planet, which was detected via radial velocity. The inner transiting planet, HATS-59b, is on an eccentric orbit with e=0.129+/- 0.049, orbiting a V=13.951+/- 0.030 ma…

2018 The Astronomical Journal
Gaia 6
The molecular H2 and stellar discs in the nuclear region of NGC 4258
DOI: 10.1093/mnras/stx2448 Bibcode: 2018MNRAS.473.2198M

Steiner, J. E.; Menezes, R. B.; da Silva, Patrícia

NGC 4258 is an SABbc Seyfert galaxy, located at a distance of 7.2 ± 0.3 Mpc. This object is well known by its nearly edge-on molecular nuclear disc, located between 0.16 and 0.28 pc from the nucleus, whose H2O maser emission allows a very precise measurement of the central supermassive black hole mass (M(maser) = 3.78 ± 0.01…

2018 Monthly Notices of the Royal Astronomical Society
eHST 6
Searching for new young stars in the Northern hemisphere: the Pisces moving group
DOI: 10.1093/mnras/stx2252 Bibcode: 2018MNRAS.473.2465B

Jeffries, R. D.; Binks, A. S.; Ward, J. L.

Using the kinematically unbiased technique described in Binks, Jeffries & Maxted (2015), we present optical spectra for a further 122 rapidly rotating (rotation periods <6 d), X-ray active FGK stars, selected from the SuperWASP survey. We identify 17 new examples of young, probably single stars with ages of <200 Myr and provide additiona…

2018 Monthly Notices of the Royal Astronomical Society
AKARI Gaia 6
The strength of ice-saturated extraterrestrial rock analogs
DOI: 10.1016/j.icarus.2018.06.016 Bibcode: 2018Icar..315...61A

Seager, Sara; Atkinson, Jared; Durham, William B.

In situ resource utilization (ISRU) activities have been identified by the National Research Council as one of the most important scientific endeavors of the coming decade. The failure of the MUPUS-PEN experiment on Rosetta's Philae lander to penetrate the surface of comet 67P demands knowledge of the mechanical properties of extraterrestrial mate…

2018 Icarus
Rosetta 6
Kinematics of outer halo globular clusters: M 75 and NGC 6426
DOI: 10.1051/0004-6361/201833110 Bibcode: 2018A&A...616A..74K

Hanke, Michael; Kacharov, Nikolay; Koch, Andreas

Globular clusters (GCs) and their dynamic interactions with the Galactic components provide an important insight into the structure and formation of the early Milky Way. We present a kinematic study of two outer halo GCs based on a combination of VLT/FORS2, VLT/FLAMES, and Magellan/MIKE low- and high-resolution spectroscopy of 32 and 27 member sta…

2018 Astronomy and Astrophysics
Gaia 6