Search Publications

Variations of the Galactic Cosmic Rays in the Recent Solar Cycles
DOI: 10.3847/1538-4365/abf936 Bibcode: 2021ApJS..254...37F

Zhao, Lingling; Fu, Shuai; Zhang, Xiaoping +1 more

In this paper, we study the Galactic cosmic-ray (GCR) variations over the solar cycles 23 and 24, with measurements from NASA's Advanced Composition Explorer/Cosmic Ray Isotope Spectrometer instrument and the ground-based neutron monitors (NMs). The results show that the maximum GCR intensities of heavy nuclei (5 ≤ Z ≤ 28, 50∼500 MeV nuc-1

2021 The Astrophysical Journal Supplement Series
SOHO 26
Orbits of 152 globular clusters of the MilkyWay galaxy constructed from Gaia DR2
DOI: 10.1088/1674-4527/21/7/173 Bibcode: 2021RAA....21..173B

Bajkova, Anisa Talgatovna; Bobylev, Vadim Vadimovich

We present orbits and their properties for 152 globular clusters of the Milky Way galaxy obtained using average Gaia DR2 proper motions and other astrometric data from the list of Vasiliev. For orbital integration we have applied the axisymmetric model of the Galactic potential based on the Navarro-Frenk- White dark halo, and modified by Bajkova &…

2021 Research in Astronomy and Astrophysics
Gaia 25
The Milky Way's bar structural properties from gravitational waves
DOI: 10.1093/mnras/staa3457 Bibcode: 2021MNRAS.500.4958W

Korol, Valeriya; Rossi, Elena M.; D'Onghia, Elena +1 more

The Laser Interferometer Space Antenna (LISA) will enable Galactic gravitational wave (GW) astronomy by individually resolving >104 signals from double white dwarf (DWD) binaries throughout the Milky Way. Since GWs are unaffected by stellar crowding and dust extinction unlike optical observations of the Galactic plane, in this work, …

2021 Monthly Notices of the Royal Astronomical Society
Gaia 25
R-process-rich Stellar Streams in the Milky Way
DOI: 10.3847/1538-4357/abea1a Bibcode: 2021ApJ...912...52G

Roederer, Ian U.; Frebel, Anna; Ji, Alexander P. +3 more

We present high-resolution Magellan/MIKE spectra of 22 bright (9 < V < 13.5) metal-poor stars (-3.18 < [Fe/H] < -1.37) in three different stellar streams, the Helmi debris stream, the Helmi trail stream, and the ω Centauri progenitor stream. We augment our Helmi debris sample with results for 10 stars by Roederer et al. for a total of …

2021 The Astrophysical Journal
Gaia 25
Systematics and Consequences of Comet Nucleus Outgassing Torques
DOI: 10.3847/1538-3881/abf09c Bibcode: 2021AJ....161..261J

Jewitt, David

Anisotropic outgassing from comets exerts a torque sufficient to rapidly change the angular momentum of the nucleus, potentially leading to rotational instability. Here, we use empirical measures of spin changes in a sample of comets to characterize the torques, and to compare them with expectations from a simple model. Both the data and the model…

2021 The Astronomical Journal
eHST 25
Rotation periods for cool stars in the open cluster NGC 3532. The transition from fast to slow rotation
DOI: 10.1051/0004-6361/202140894 Bibcode: 2021A&A...652A..60F

Strassmeier, K. G.; Barnes, S. A.; James, D. J. +1 more

Context. A very rich cluster intermediate in age between the Pleiades (150 Myr) and the Hyades (600 Myr) is needed to probe the rotational evolution, especially the transition between fast and slow rotation that occurs between the two ages.
Aims: We study the rich 300 Myr-old open cluster NGC 3532 to probe this important transition and to pro…

2021 Astronomy and Astrophysics
Gaia 25
ALMA Observations of the Sub-kpc Structure of the Host Galaxy of a z = 6.5 Lensed Quasar: A Rotationally Supported Hyper-Starburst System at the Epoch of Reionization
DOI: 10.3847/1538-4357/ac0af4 Bibcode: 2021ApJ...917...99Y

Fan, Xiaohui; Keeton, Charles R.; Walter, Fabian +11 more

We report Atacama Large Millimeter/Submillimeter Array (ALMA) observations of the dust continuum and [C II] emission of the host galaxy of J0439+1634, a gravitationally lensed quasar at z = 6.5. Gravitational lensing boosts the source-plane resolution to ~0"15 (~0.8 kpc). The lensing model derived from the ALMA data is consistent with the fiducial…

2021 The Astrophysical Journal
eHST 25
Data Mining Reconstruction of Magnetotail Reconnection and Implications for Its First-Principle Modeling
DOI: 10.3389/fphy.2021.644884 Bibcode: 2021FrP.....9...90S

Sitnov, Mikhail; Stephens, Grant; Motoba, Tetsuo +1 more

Magnetic reconnection is a fundamental process providing topological changes of the magnetic field, reconfiguration of space plasmas and release of energy in key space weather phenomena, solar flares, coronal mass ejections and magnetospheric substorms. Its multiscale nature is difficult to study in observations because of their sparsity. Here we …

2021 Frontiers in Physics
Cluster 25
A Galactic survey of radio jets from massive protostars
DOI: 10.1093/mnras/stab747 Bibcode: 2021MNRAS.504..338P

Lumsden, S. L.; Purser, S. J. D.; Hoare, M. G. +1 more

In conjunction with a previous southern-hemisphere work, we present the largest radio survey of jets from massive protostars to date with high-resolution (~0.04 arcsec) Jansky Very Large Array observations towards two subsamples of massive star-forming regions of different evolutionary statuses: 48 infrared-bright, massive, young, stellar objects …

2021 Monthly Notices of the Royal Astronomical Society
AKARI 25
TESS Asteroseismology of α Mensae: Benchmark Ages for a G7 Dwarf and Its M Dwarf Companion
DOI: 10.3847/1538-4357/ac1269 Bibcode: 2021ApJ...922..229C

Butler, R. Paul; Chaplin, William J.; Stassun, Keivan G. +27 more

Asteroseismology of bright stars has become increasingly important as a method to determine the fundamental properties (in particular ages) of stars. The Kepler Space Telescope initiated a revolution by detecting oscillations in more than 500 main-sequence and subgiant stars. However, most Kepler stars are faint and therefore have limited constrai…

2021 The Astrophysical Journal
Gaia 25