Search Publications

Spectra of Cosmic-Ray Sodium and Aluminum and Unexpected Aluminum Excess
DOI: 10.3847/1538-4357/ac7443 Bibcode: 2022ApJ...933..147B

Jóhannesson, G.; Moskalenko, I. V.; Porter, T. A. +11 more

Since its launch, the Alpha Magnetic Spectrometer-02 (AMS-02) has delivered outstanding quality measurements of the spectra of cosmic-ray (CR) species, $\bar{p}$ , e ±, and nuclei (H-Si, Fe), which resulted in a number of breakthroughs. The most recent AMS-02 result is the measurement of the spectra of CR sodium and aluminum up to ~2 TV…

2022 The Astrophysical Journal
Ulysses 7
Discovery of Year-scale Time Variability from Thermal X-Ray Emission in Tycho's Supernova Remnant
DOI: 10.3847/1538-4357/ac94cf Bibcode: 2022ApJ...940..105M

Yamaguchi, Hiroya; Uchida, Hiroyuki; Tsuru, Takeshi Go +2 more

Mechanisms of particle heating are crucial to understanding the shock physics in supernova remnants (SNRs). However, there has been little information on time variabilities of thermalized particles so far. Here, we present a discovery of a gradually brightening thermal X-ray emission found in the Chandra data of Tycho's SNR obtained during 2000-20…

2022 The Astrophysical Journal
eHST 7
Core orientations and magnetic fields in isolated molecular clouds
DOI: 10.1093/mnras/stac2487 Bibcode: 2022MNRAS.517.1138S

Soam, Archana; Lee, Chang Won; Sharma, Ekta +2 more

Molecular clouds are sites of star formation. Magnetic fields are believed to play an important role in their dynamics and shaping morphology. We aim to study any possible correlation that might exist between the magnetic fields orientation inside the clouds and the magnetic fields at envelope scales and their connection with respect to the observ…

2022 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 7
Polarization from Aligned Dust Grains in the β Pic Debris Disk
DOI: 10.3847/1538-4357/ac6023 Bibcode: 2022ApJ...930...49H

Hughes, A. Meredith; Hull, Charles L. H.; Le Gouellec, Valentin J. M. +8 more

We present 870 µm Atacama Large Millimeter/submillimeter Array polarization observations of thermal dust emission from the iconic, edge-on debris disk β Pic. While the spatially resolved map does not exhibit detectable polarized dust emission, we detect polarization at the ~3σ level when averaging the emission across the entire disk. The cor…

2022 The Astrophysical Journal
Gaia 7
An Optical Spectrum of the Diffuse Galactic Light from BOSS and IRIS
DOI: 10.3847/1538-4357/ac6efc Bibcode: 2022ApJ...932..112C

Hensley, Brandon S.; Brandt, Timothy D.; Draine, Bruce T. +2 more

We present a spectrum of the diffuse Galactic light (DGL) between 3700 and 10,000 Å, obtained by correlating optical sky intensity with far-infrared dust emission. We use nearly 250,000 blank-sky spectra from BOSS/SDSS-III together with IRIS-reprocessed maps from the IRAS satellite. The larger sample size compared to SDSS-II results in a factor-of…

2022 The Astrophysical Journal
Gaia 7
Observations of cross scale energy transfer in the inner heliosphere by Parker Solar Probe
DOI: 10.1007/s41614-022-00097-x Bibcode: 2022RvMPP...6...41P

Parashar, Tulasi N.; Matthaeus, William H.

The solar wind, a continuous flow of plasma from the sun, not only shapes the near Earth space environment but also serves as a natural laboratory to study plasma turbulence in conditions that are not achievable in the lab. Starting with the Mariners, for more than five decades, multiple space missions have enabled in-depth studies of solar wind t…

2022 Reviews of Modern Plasma Physics
Ulysses 7
In the Trenches of the Solar-Stellar Connection. VI. Total EclipSS
DOI: 10.3847/1538-4365/ac8cfc Bibcode: 2022ApJS..263...41A

Buzasi, Derek; Ayres, Thomas

The Ecliptic poles Stellar Survey (EclipSS; 2018-2019) collected Hubble Space Telescope/Cosmic Origins Spectrograph (COS) 1150-1420 Å spectra of 49 FGK dwarfs at high ecliptic latitudes. These regions are favored by the scanning programs of the Transiting Exoplanet Survey Satellite (TESS; high-precision optical light curves) and Extended Roentgen …

2022 The Astrophysical Journal Supplement Series
Gaia XMM-Newton eHST 7
Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate
DOI: 10.1093/pasj/psab112 Bibcode: 2022PASJ...74...92T

Izumiura, Hideyuki; Sato, Bun'ei; Yoshida, Michitoshi +9 more

We report the detection of radial velocity (RV) variations in nine evolved G- and K-type giant stars. The observations were conducted at Okayama Astrophysical Observatory. Planets or planet candidates can best explain these regular variations. However, a coincidence of near 280 d variability among five of them prevents us from fully ruling out ste…

2022 Publications of the Astronomical Society of Japan
Gaia 7
A Vindication of the RR Lyrae Fourier Light Curve Decomposition for the Calculation of Metallicity and Distance in Globular Clusters
DOI: 10.22201/ia.01851101p.2022.58.02.08 Bibcode: 2022RMxAA..58..257A

Arellano Ferro, A.

We report the mean metallicity and absolute magnitude of RR Lyrae stars in a sample of 37 globular clusters, calculated via the Fourier decomposition of their light curves and ad hoc semi-empirical calibrations, in an unprecedented homogeneous approach. This enabled a new discussion of the metallicity dependence of the horizontal branch (HB) lumin…

2022 Revista Mexicana de Astronomia y Astrofisica
Gaia 7
A White Dwarf-Main-sequence Binary Unveiled by Time-domain Observations from LAMOST and TESS
DOI: 10.3847/1538-4357/ac853f Bibcode: 2022ApJ...936...33Z

Liu, Jifeng; Zong, Weikai; Bai, Yu +16 more

We report a single-lined white dwarf-main-sequence binary system, LAMOST J172900.17+652952.8, which is discovered by the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST)'s medium-resolution time-domain surveys. The radial-velocity semi-amplitude and orbital period of the optical visible star are measured by using follow-up observ…

2022 The Astrophysical Journal
Gaia 7