Search Publications

The Massive and Distant Clusters of WISE Survey. VI. Stellar Mass Fractions of a Sample of High-redshift Infrared-selected Clusters
DOI: 10.3847/1538-4357/ab12d7 Bibcode: 2019ApJ...878...72D

Gupta, Nikhel; Eisenhardt, Peter R. M.; Gonzalez, Anthony H. +17 more

We present measurements of the stellar mass fractions ({f}\star ) for a sample of high-redshift (0.93 ≤ z ≤ 1.32) infrared-selected galaxy clusters from the Massive and Distant Clusters of WISE Survey (MaDCoWS) and compare them to the stellar mass fractions of Sunyaev-Zel’dovich (SZ) effect-selected clusters in a similar mass and redshi…

2019 The Astrophysical Journal
Gaia 12
On the photometric signature of fast rotators
DOI: 10.1093/mnras/stz1767 Bibcode: 2019MNRAS.488..696G

Girardi, Léo; Marigo, Paola; Bellini, Andrea +4 more

Rapidly rotating stars have been recently recognized as having a major role in the interpretation of colour-magnitude diagrams of young and intermediate-age star clusters in the Magellanic Clouds and in the Milky Way. In this work, we evaluate the distinctive spectra and distributions in colour-colour space that follow from the presence of a subst…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 12
Spectroscopic Orbits of Subsystems in Multiple Stars. V.
DOI: 10.3847/1538-3881/aafe00 Bibcode: 2019AJ....157...91T

Tokovinin, Andrei

Spectroscopic orbits are determined for inner subsystems in nine stellar hierarchies (HIP 2863, 4974, 8353, 28796, 35261, 92929, 115272, 115552, and 117596). Their periods range from 2.5 to 312 days. For each system, estimates of masses, orbital inclination, and other parameters are given.

2019 The Astronomical Journal
Gaia Hipparcos 12
Transition-region explosive events produced by plasmoid instability
DOI: 10.1088/1674-4527/19/5/67 Bibcode: 2019RAA....19...67L

Li, Dong

Magnetic reconnection is thought to be a key process in most solar eruptions. Thanks to highresolution observations and simulations, the studied scale of the reconnection process has become smaller and smaller. Spectroscopic observations show that the reconnection site can be very small, which always exhibits a bright core and two extended wings w…

2019 Research in Astronomy and Astrophysics
IRIS 12
Recognition of M-type stars in the unclassified spectra of LAMOST DR5 using a hash-learning method
DOI: 10.1093/mnras/stz458 Bibcode: 2019MNRAS.485.2167G

Luo, A. -L.; Chen, J. -J.; Du, B. +6 more

Our study aims to recognize M-type stars which are classified as `UNKNOWN' due to poor quality in the Large sky Area Multi-Object fiber Spectroscopic Telescope (LAMOST) DR5 V1. A binary nonlinear hashing algorithm based on Multi-Layer Pseudo-Inverse Learning (ML-PIL) is proposed to effectively learn spectral features for M-type-star detection, whi…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 12
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