Search Publications

Assessing Martian bedrock mineralogy through "windows" in the dust using near-infrared and thermal infrared remote sensing
DOI: 10.1016/j.icarus.2019.01.019 Bibcode: 2019Icar..324...15L

Horgan, Briony; Bell, James F., III; Lai, Jason C. +1 more

Much of Mars' surface is mantled by bright dust, which masks the spectral features used to interpret the mineralogy of the underlying bedrock. Despite the wealth of near-infrared (NIR) and thermal infrared (TIR) data returned from orbiting spacecraft in recent decades, the detailed bedrock composition of approximately half of the Martian surface r…

2019 Icarus
MEx 4
Multiwavelength observations of the triple-peaked AGN Mrk 622
DOI: 10.1093/mnras/stz2884 Bibcode: 2019MNRAS.490.5521B

Jiménez-Bailón, E.; Binette, L.; González-Martín, O. +8 more

A detailed multiwavelength study of the properties of the triple-peaked active galactic nucleus (AGN) Mrk 622 showing different aspects of the nuclear emission region is presented. Radio, near- and mid-infrared, optical, and X-ray data have been considered for the analysis. In the optical, the WHAN diagnostic diagrams show that the three nuclear p…

2019 Monthly Notices of the Royal Astronomical Society
eHST 4
On the age of the Beagle secondary asteroid family
DOI: 10.1016/j.pss.2018.08.004 Bibcode: 2019P&SS..166...90C

Carruba, V.

The Beagle family is a C-type subgroup of the Themis family, in the outer main belt. Previous works suggested that it could be younger than 20 Myr and a possible source for the dust in the i ≃1.4 α zodiacal dust band. Here we took advantage of a much larger database for Beagle family members to revisit previous age estimates of this gr…

2019 Planetary and Space Science
AKARI 4
Transit timing variations, radial velocities, and long-term dynamical stability of the system Kepler-410
DOI: 10.1093/mnras/stz305 Bibcode: 2019MNRAS.484.4352G

Kabáth, Petr; Skarka, Marek; Šubjak, Ján +6 more

Transit timing variations (TTVs) of Kepler-410Ab were already reported in a few papers. Their semi-amplitude is about 14.5 min. In our previous paper, we found that the TTVs could be caused by the presence of a stellar companion in this system. Our main motivation for this paper was to investigate variation in a radial-velocity (RV) curve generate…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
Astroinformatics-based search for globular clusters in the Fornax Deep Survey
DOI: 10.1093/mnras/stz2801 Bibcode: 2019MNRAS.490.4080A

Paolillo, M.; Peletier, R.; Hilker, M. +15 more

In the last years, Astroinformatics has become a well-defined paradigm for many fields of Astronomy. In this work, we demonstrate the potential of a multidisciplinary approach to identify globular clusters (GCs) in the Fornax cluster of galaxies taking advantage of multiband photometry produced by the VLT Survey Telescope using automatic self-adap…

2019 Monthly Notices of the Royal Astronomical Society
eHST 4
A New Type of Jet in a Polar Limb of the Solar Coronal Hole
DOI: 10.3847/2041-8213/ab4799 Bibcode: 2019ApJ...884L..38C

Moon, Yong-Jae; Cho, Kyung-Suk; Kim, Yeon-Han +3 more

A new type of chromospheric jet in a polar limb of a coronal hole is discovered in the Ca II filtergram of the Solar Optical Telescope on board the Hinode. We identify 30 jets in a filtered Ca II movie with a duration of 53 minutes. The average speed at their maximum heights is found to be 132 ± 44 km s-1 ranging from 57 to 264 km s

2019 The Astrophysical Journal
Hinode 4
Study of Interplanetary CMEs/Shocks During Solar Cycle 24 Using Drag-Based Model: The Role of Solar Wind
DOI: 10.1007/s11207-019-1432-8 Bibcode: 2019SoPh..294...47S

Shanmugaraju, A.; Vršnak, Bojan; Suresh, K. +2 more

In this paper we analyze a set of 27 fast interplanetary coronal mass ejections (ICMEs) observed during the period January 2010 - December 2013 in Solar Cycle 24. The arrivals of interplanetary shocks and CMEs at 1 AU are found from OMNI spacecraft high resolution data and their travel times are compared with Empirical Shock Arrival (ESA; Gopalswa…

2019 Solar Physics
SOHO 4
Close up observation and inversion of low-altitude ENA emissions during a substorm event
DOI: 10.1007/s11430-018-9307-x Bibcode: 2019ScChD..62.1024L

McKenna-Lawlor, Susan; Lu, Li; Balaz, Jan

During a series of substorm events on November 12 2004, the Neutral Atom Detector Unit (NUADU) flying onboard the TC-2 spacecraft observed, close to perigee, bright low-altitude Energetic Neutral Atom (ENA) emissions from both north and south poles. Through utilizing high temporal and spatial resolution data inversion techniques we present here a …

2019 Science China Earth Sciences
DoubleStar 4
The Difference Between Isolated Flux Transfer Events and Flux Transfer Event Cascades
DOI: 10.1029/2019JA026629 Bibcode: 2019JGRA..124.7850K

Karlsson, T.; Kullen, A.; Thor, S.

This flux transfer event (FTE) study is based on 984 FTEs originally identified by Wang et al. (2005, https://doi:10.1029/2005JA011150) in Cluster data. Due to Cluster's orbit, the FTE list exclusively contains events detected at the high-latitude dayside magnetopause and low-latitude flanks. The focu…

2019 Journal of Geophysical Research (Space Physics)
Cluster 4
Two Circumstellar Nebulae Discovered with the Wide-field Infrared Survey Explore and Their Massive Central Stars
DOI: 10.3847/1538-3881/aaf56c Bibcode: 2019AJ....157...53G

Grebel, Eva K.; Castro, Norberto; Gvaramadze, Vasilii V. +1 more

We report the discovery of two mid-infrared nebulae in the northern hemisphere with the Wide-field Infrared Survey Explorer and the results of optical spectroscopy of their central stars, BD+60° 2668 (composed of two components, separated from each other by ≈3 arcsec) and ALS 19653, with the Calar Alto 3.5 m telescope and the Southern African Larg…

2019 The Astronomical Journal
Gaia 4