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XMM-Newton Detection and Spectrum of the Second Fastest Spinning Pulsar PSR J0952-0607
DOI: 10.3847/1538-4357/ab3578 Bibcode: 2019ApJ...882..128H

Ho, Wynn C. G.; Heinke, Craig O.; Chugunov, Andrey I.

With a spin frequency of 707 Hz, PSR J0952-0607 is the second fastest spinning pulsar known. It was discovered in radio by LOFAR in 2017 at an estimated distance of either 0.97 or 1.74 kpc and has a low-mass companion with a 6.42 hr orbital period. We report the discovery of the X-ray counterpart of PSR J0952-0607 using XMM-Newton. The X-ray spect…

2019 The Astrophysical Journal
XMM-Newton 13
Evolution of Coronal Mass Ejection Properties in the Inner Heliosphere: Prediction for the Solar Orbiter and Parker Solar Probe
DOI: 10.3847/1538-4357/ab4126 Bibcode: 2019ApJ...884..179A

Poedts, Stefaan; Lugaz, Noé; Al-Haddad, Nada +3 more

The evolution of the magnetic field and plasma quantities inside a coronal mass ejection (CME) with distance are known from statistical studies using data from 1 au monitors, planetary missions, Helios, and Ulysses. This does not cover the innermost heliosphere, below 0.29 au, where no data are yet publicly available. Here, we describe the evoluti…

2019 The Astrophysical Journal
SolarOrbiter 13
Acceleration of protons and heavy ions to suprathermal energies during dipolarizations in the near-Earth magnetotail
DOI: 10.5194/angeo-37-549-2019 Bibcode: 2019AnGeo..37..549M

Grigorenko, Elena E.; Kronberg, Elena A.; Daly, Patrick W. +2 more

In this work we present an analysis of the dynamics of suprathermal ions of different masses (H+, He+, O+) during prolonged dipolarizations in the near-Earth magnetotail (X>-17RE) according to Cluster/RAPID observations in 2001-2005. All dipolarizations from our database were associated with fast flow…

2019 Annales Geophysicae
Cluster 13
Chemical abundances of open clusters from high-resolution infrared spectra - I. NGC 6940
DOI: 10.1093/mnras/stz727 Bibcode: 2019MNRAS.485.4625B

Sneden, C.; Pilachowski, C. A.; Mace, G. N. +8 more

We present near-infrared spectroscopic analysis of 12 red giant members of the Galactic open cluster NGC 6940. High-resolution (R ≃ 45 000) and high-signal-to-noise ratio (S/N > 100) near-infrared H- and K-band spectra were gathered with the Immersion Grating Infrared Spectrograph (IGRINS) on the 2.7-m Smith Telescope at McDonald Observatory. W…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 13
Energetic Oxygen and Sulfur Charge States in the Outer Jovian Magnetosphere: Insights From the Cassini Jupiter Flyby
DOI: 10.1029/2019GL085185 Bibcode: 2019GeoRL..4611709A

Wilson, R. J.; Krimigis, S. M.; Mitchell, D. G. +10 more

On 10 January 2001, Cassini briefly entered into the magnetosphere of Jupiter, en route to Saturn. During this excursion into the Jovian magnetosphere, the Cassini Magnetosphere Imaging Instrument/Charge-Energy-Mass Spectrometer detected oxygen and sulfur ions. While Charge-Energy-Mass Spectrometer can distinguish between oxygen and sulfur charge …

2019 Geophysical Research Letters
Cassini 13
Graphene oxide nanoparticles in the interstellar medium
DOI: 10.1093/mnrasl/slz131 Bibcode: 2019MNRAS.490L..17S

Sarre, P. J.

Dust particles play a major role in the formation, evolution and chemistry of interstellar clouds, stars, and planetary systems. Commonly identified forms include amorphous and crystalline carbon-rich particles and silicates. Also present in many astrophysical environments are polycyclic aromatic hydrocarbons (PAHs), detected through their infrare…

2019 Monthly Notices of the Royal Astronomical Society
ISO 13
Resolving the Interstellar Medium in Ultraluminous Infrared QSO Hosts with ALMA
DOI: 10.3847/1538-4357/ab50be Bibcode: 2019ApJ...887...24T

Kohno, Kotaro; Daddi, Emanuele; Gao, Yu +8 more

We present ALMA observations of the CO(1-0) line and 3 mm continuum emission in eight ultraluminous infrared (IR) quasi-stellar objects (QSOs) at z = 0.06-0.19. All eight IR QSO hosts are clearly resolved in their CO molecular gas emission with a median source size of 3.2 kpc, and seven out of eight sources are detected in 3 mm continuum, which is…

2019 The Astrophysical Journal
eHST 13
Compact star-forming galaxies preferentially quenched to become PSBs in z < 1 clusters
DOI: 10.1093/mnras/sty2840 Bibcode: 2019MNRAS.482.1640S

Simpson, Chris; Wild, Vivienne; Almaini, Omar +5 more

We analyse the structure of galaxies with high specific star formation rate (SSFR) in cluster and field environments in the redshift range 0.5 < z < 1.0. Recent studies have shown that these galaxies are strongly depleted in dense environments due to rapid environmental quenching, giving rise to post-starburst galaxies (PSBs). We use effecti…

2019 Monthly Notices of the Royal Astronomical Society
eHST 13
HST/COS Observations of the Warm Ionized Gaseous Halo of NGC 891
DOI: 10.3847/1538-4357/ab17df Bibcode: 2019ApJ...876..101Q

Bregman, Joel N.; Qu, Zhijie; Hodges-Kluck, Edmund J.

The metallicity of galactic gaseous halos provides insights into accretion and feedback of galaxies. The nearby edge-on galaxy NGC 891 has a multicomponent gaseous halo and a background active galactic nucleus (AGN; LQAC 035+042 003) projected 5 kpc above the disk near the minor axis. Against the UV continuum of this AGN, we detect lines from 13 i…

2019 The Astrophysical Journal
eHST 13
Discovery statistics and 1/a distribution of long-period comets detected during 1801-2017
DOI: 10.1093/mnras/stz025 Bibcode: 2019MNRAS.484.3463K

Dybczyński, Piotr A.; Królikowska, Małgorzata

For the last two decades, we have been observing a huge increase in discoveries of long-period comets (LPCs), especially those with large perihelion distances. We collected data for a full sample of LPCs discovered during 1801-2017, including their osculating orbits, discovery moments (to study the discovery distances) and original semimajor axes …

2019 Monthly Notices of the Royal Astronomical Society
SOHO 13