Search Publications

New Candidate Planetary Nebulae in Galactic Globular Clusters from the VVV Survey
DOI: 10.3847/2041-8213/ab4424 Bibcode: 2019ApJ...884L..15M

Minniti, Dante; Dias, Bruno; Gómez, Matías +2 more

Only four globular cluster planetary nebulae (GCPN) are known so far in the Milky Way. About 50 new globular clusters have been recently discovered toward the Galactic bulge. We present a search for planetary nebulae within 3‧ of the new globular clusters, revealing the identification of new candidate GCPN. These possible associations are PN SB 2 …

2019 The Astrophysical Journal
Gaia 12
Detection of spike-like structures near the front of type-II bursts
DOI: 10.1051/0004-6361/201834982 Bibcode: 2019A&A...624A..76A

Hillaris, A.; Preka-Papadema, P.; Moussas, X. +6 more


Aims: We examine high time resolution dynamic spectra for fine structures in type II solar radio bursts
Methods: We used data obtained with the acousto-optic spectrograph receiver of the Artemis-JLS (ARTEMIS-IV) solar radio spectrograph in the 450-270 MHz range at 10 ms cadence and identified more than 600 short, narrowband features. The…

2019 Astronomy and Astrophysics
SOHO 12
Detecting the orbital motion of nearby supermassive black hole binaries with Gaia
DOI: 10.1103/PhysRevD.100.103016 Bibcode: 2019PhRvD.100j3016D

Loeb, Abraham; D'Orazio, Daniel J.

We show that a 10-yr Gaia mission could astrometrically detect the orbital motion of ∼1 subparsec separation supermassive black hole binary in the heart of nearby, bright active galactic nuclei (AGN). Candidate AGN lie out to a redshift of z =0.02 and in the V-band magnitude range 10 ≲mV≲13 . The distribution of detectable binary masses…

2019 Physical Review D
Gaia 12
2003-2018 Monitoring of the Crab Nebula Polarization in Hard X-Rays with INTEGRAL SPI
DOI: 10.3847/1538-4357/ab3422 Bibcode: 2019ApJ...882..129J

Jourdain, E.; Roques, J. -P.

We analyzed 16 yr of observations dedicated to the Crab (pulsar + nebula) with the SPectrometer on International Gamma-Ray Astrophysics Laboratory instrument to investigate its polarization properties. We find that the source presents a substantially polarized emission (PF = 24%) in the hard X-ray domain, with the electric vector aligned with the …

2019 The Astrophysical Journal
INTEGRAL 12
Radical-assisted polymerization in interstellar ice analogues: formyl radical and polyoxymethylene
DOI: 10.1093/mnras/stz879 Bibcode: 2019MNRAS.486.1953B

Duvernay, F.; Danger, G.; Chiavassa, T. +5 more

We present new laboratory experiments on the low-temperature formation of complex organic molecules (COMs) such as polyoxymethylene (POM), glycolaldehyde, ethylene glycol, and possibly glyceraldehyde and glycerol through radical-induced reactivity from vacuum ultraviolet (VUV) photolysis of formaldehyde in Ar and Xe matrices. The radical reactivit…

2019 Monthly Notices of the Royal Astronomical Society
Rosetta 12
Active Region Modulation of Coronal Hole Solar Wind
DOI: 10.3847/1538-4357/ab5586 Bibcode: 2019ApJ...887..146M

Wicks, Robert T.; Long, David M.; Harra, Louise K. +4 more

Active regions (ARs) are a candidate source of the slow solar wind (SW), the origins of which are a topic of ongoing research. We present a case study that examines the processes by which SW is modulated in the presence of an AR in the vicinity of the SW source. We compare properties of SW associated with a coronal hole (CH)-quiet Sun boundary to …

2019 The Astrophysical Journal
Hinode 12
Quantifying the Propagation of Fast Coronal Mass Ejections from the Sun to Interplanetary Space by Combining Remote Sensing and Multi-point In Situ Observations
DOI: 10.3847/1538-4357/ab379b Bibcode: 2019ApJ...882..122Z

Wang, Rui; Liu, Ying D.; Hu, Huidong +1 more

In order to have a comprehensive view of the propagation and evolution of coronal mass ejections (CMEs) from the Sun to deep interplanetary space beyond 1 au, we carry out a kinematic analysis of seven CMEs in solar cycle 23. The events are required to have coordinated coronagraph observations, interplanetary type II radio bursts, and multi-point …

2019 The Astrophysical Journal
SOHO Ulysses 12
LISA Pathfinder mission extension: A feasibility analysis
DOI: 10.1016/j.asr.2019.02.035 Bibcode: 2019AdSpR..63.3863D

Rasotto, Mirco; Renk, Florian; Dei Tos, Diogene A. +1 more

A proposed mission extension for LISA Pathfinder involved redirecting the probe to the Sun-Earth gravitational saddle point. Realistic models for both space and ground segments were used to carry out a number of analyses for trajectory design, orbit determination, and navigation cost. In this work, we present the methods that allow assessing the f…

2019 Advances in Space Research
LISAPathfinder 12
Interpretation through experimental simulations of phase functions revealed by Rosetta in 67P/Churyumov-Gerasimenko dust coma
DOI: 10.1051/0004-6361/201834894 Bibcode: 2019A&A...630A..20L

Lasue, J.; Fulle, M.; Bertini, I. +3 more

Context. The dust-brightness phase curves that have been measured by the OSIRIS cameras on board the Rosetta spacecraft within the coma of comet 67P/Churyumov-Gerasimenko (67P) present a remarkable flattened u-shape.
Aims: Our goal is to compare these phase curves with those of tentatively analog dust samples to assess the key dust properties…

2019 Astronomy and Astrophysics
Rosetta 12
Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z > 1
DOI: 10.3847/1538-4357/ab521e Bibcode: 2019ApJ...887...76K

Huang, Xiaosheng; Rubin, David; Perlmutter, Saul +5 more

We present a detailed high-resolution weak-lensing study of SPT-CL J2106-5844 at z = 1.132, claimed to be the most massive system discovered at z > 1 in the South Pole Telescope Sunyaev-Zel’dovich survey. Based on the deep imaging data from the Advanced Camera for Surveys and Wide Field Camera 3 on board the Hubble Space Telescope, we find that…

2019 The Astrophysical Journal
eHST 12