Search Publications

Evidence for a Rotational Component in the Circumgalactic Medium of Nearby Galaxies
DOI: 10.3847/1538-4357/ab9905 Bibcode: 2020ApJ...897..151F

Wakker, Bart P.; French, David M.

We present results of a study comparing the relative velocity of Lyα absorbers to the rotation velocity of nearby galaxy disks in the local universe (z ≤ 0.03). We have obtained rotation curves via long-slit spectroscopy of eight galaxies with the Southern African Large Telescope, and combine this data set with an additional 16 galaxies with data …

2020 The Astrophysical Journal
eHST 14
Hierarchical star formation in nearby galaxies
DOI: 10.1051/0004-6361/202038970 Bibcode: 2020A&A...644A.101R

Baume, G.; Rodríguez, M. J.; Feinstein, C.


Aims: The purpose of this work is to study the properties of the spatial distribution of the young population in three nearby galaxies in order to better understand the first stages of star formation.
Methods: We used ACS/HST photometry and the "path-linkage criterion" in order to obtain a catalog of young stellar groups (YSGs) in the ga…

2020 Astronomy and Astrophysics
eHST 14
Probing the nuclear and circumnuclear properties of NGC 6300 using X-ray observations
DOI: 10.1093/mnras/staa2552 Bibcode: 2020MNRAS.499.5396J

Naik, Sachindra; Jana, Arghajit; Chatterjee, Arka +3 more

We present the results obtained from a detailed X-ray timing and spectral analysis of the Seyfert 2 galaxy NGC 6300 by using observations from the Suzaku observatory, theChandra X-ray Observatory and the Nuclear Spectroscopic Telescope Array(NuSTAR) mission between 2007 and 2016. We calculate the variance and the rms fractional variability of the …

2020 Monthly Notices of the Royal Astronomical Society
Suzaku 14
ASKAP reveals giant radio halos in two merging SPT galaxy clusters
DOI: 10.1017/pasa.2020.34 Bibcode: 2020PASA...37...40W

Johnston-Hollitt, Melanie; Akamatsu, Hiroki; Hodgson, Torrance +4 more

Early science observations from the Australian Square Kilometre Array Pathfinder (ASKAP) have revealed clear signals of diffuse radio emission associated with two clusters detected by the South Pole Telescope via their Sunyaev Zel'dovich signal: SPT CLJ0553-3342 (MACS J0553.4-3342) and SPT CLJ0638-5358 (Abell S0592) are both high-mass lensing clus…

2020 Publications of the Astronomical Society of Australia
eHST 14
Chemically Peculiar A and F Stars with Enhanced s-process and Iron-peak Elements: Stellar Radiative Acceleration at Work
DOI: 10.3847/1538-4357/ab99a5 Bibcode: 2020ApJ...898...28X

Ting, Yuan-Sen; Rix, Hans-Walter; Zhang, Meng +6 more

We present ≳15,000 metal-rich ([Fe/H] > -0.2 dex) A and F stars whose surface abundances deviate strongly from solar abundance ratios and cannot plausibly reflect their birth material composition. These stars are identified by their high [Ba/Fe] abundance ratios ([Ba/Fe] > 1.0 dex) in the LAMOST DR5 spectra analyzed by Xiang et al. They are …

2020 The Astrophysical Journal
Gaia 14
A Catalog of Bipolar Active Regions Violating the Hale Polarity Law, 1989 - 2018
DOI: 10.1007/s11207-020-01734-9 Bibcode: 2020SoPh..295..165Z

Zhukova, Anastasiya; Sokoloff, Dmitry; Abramenko, Valentina +1 more

There is no list of bipolar active regions (ARs) with reverse polarity (anti-Hale regions), although statistical investigations of such ARs (bearing the imprint of deep subphotospheric processes) are important for understanding solar-cycle mechanisms. We studied 8606 ARs from 1 January 1989 to 31 December 2018 to detect anti-Hale regions and to co…

2020 Solar Physics
SOHO 14
Chandra Monitoring of the J1809-1917 Pulsar Wind Nebula and Its Field
DOI: 10.3847/1538-4357/abaf4b Bibcode: 2020ApJ...901..157K

Pavlov, George G.; Kargaltsev, Oleg; Klingler, Noel +3 more

PSR J1809-1917 is a young (τ = 51 kyr) and energetic ( $\dot{E}=1.8\times {10}^{36}$ erg s-1) radio pulsar powering an X-ray pulsar wind nebula (PWN) that exhibits morphological variability. We report on the results of a new monitoring campaign by the Chandra X-ray Observatory (Chandra), carried out across six epochs with a ∼7 week cade…

2020 The Astrophysical Journal
Gaia XMM-Newton 14
A Rapidly Varying Red Supergiant X-Ray Binary in the Galactic Center
DOI: 10.3847/1538-4357/ab90ff Bibcode: 2020ApJ...896...32G

Gottlieb, Amy M.; Ackley, Kendall; DeWitt, Curtis +2 more

We analyzed multiwavelength observations of the previously identified Galactic center X-ray binary CXO 174528.79-290942.8 (XID 6592) and determine that the near-infrared counterpart is a red supergiant based on its spectrum and luminosity. Scutum X-1 is the only previously known X-ray binary with a red supergiant donor star and closely resembles X…

2020 The Astrophysical Journal
XMM-Newton 14
The Detection of Dust Gap-ring Structure in the Outer Region of the CR Cha Protoplanetary Disk
DOI: 10.3847/1538-4357/ab5d2b Bibcode: 2020ApJ...888...72K

Dong, Ruobing; Kataoka, Akimasa; Sitko, Michael +13 more

We observe the dust continuum at 225 GHz and CO isotopologue (12CO, 13CO, and C18O) J = 2-1 emission lines toward the CR Cha protoplanetary disk using the Atacama Large Millimeter/submillimeter Array. The dust continuum image shows a dust gap-ring structure in the outer region of the dust disk. A faint dust ring is…

2020 The Astrophysical Journal
Gaia 14
Placing limits on long-term variations in quiet-Sun irradiance and their contribution to total solar irradiance and solar radiative forcing of climate
DOI: 10.1098/rspa.2020.0077 Bibcode: 2020RSPSA.47600077L

Lockwood, Mike; Ball, William T.

Recent reconstructions of total solar irradiance (TSI) postulate that quiet-Sun variations could give significant changes to the solar power input to Earth's climate (radiative climate forcings of 0.7-1.1 W m-2 over 1700-2019) arising from changes in quiet-Sun magnetic fields that have not, as yet, been observed. Reconstructions without…

2020 Proceedings of the Royal Society of London Series A
SOHO 14