Results 31 to 40 of about 30,122 (121)

HISTORY OF STEREOLOGY

open access: yesImage Analysis and Stereology, 2017
Nowadays it is difficult to list all disciplines where stereology is applied, starting from biology and medicine, through materials science, geology and agriculture, up to military systems, biometry, meteorology, geography, physics, astronomy ...
Aneta Gądek-Moszczak
doaj   +1 more source

Spatially Resolved Galactic Winds at Cosmic Noon: Outflow Kinematics and Mass Loading in a Lensed Star-forming Galaxy at z = 1.87

open access: yesThe Astrophysical Journal
We study the spatially resolved outflow properties of CSWA13, an intermediate-mass ( M _*  = 10 ^9 M _⊙ ), gravitationally lensed star-forming galaxy at z = 1.87.
Keerthi Vasan G. C.   +15 more
doaj   +1 more source

“She would charm people with her mind’s enchantment only”. On the intellectual environment of Marianna Skórzewska, née Ciecierska, on the basis of the inventory of her book collection

open access: yesBiblioteka, 2017
Marianna Skórzewska, née Ciecierska (1741–1773), a wealthy noblewoman, wife of General Franciszek Skórzewski, shared her time between Greater Poland (palace at Margonińska Wieś) and Berlin.
Kamila Kłudkiewicz
doaj   +1 more source

Turbulent Gas-rich Disks at High Redshift: Origin of Thick Stellar Disks Through 3D “Baryon Sloshing”

open access: yesThe Astrophysical Journal
In response to recent observations from JWST and Atacama Large Millimeter Array, we explore a new class of dynamically self-consistent models that mimics a plausible progenitor of the Milky Way over a wide range of disk gas fractions, f _gas .
Joss Bland-Hawthorn   +10 more
doaj   +1 more source

Aliasing from Galactic Plane Setting in Widefield Radio Interferometry

open access: yesThe Astrophysical Journal
Measurements with widefield radio interferometers often include the near-infinite gradient between the sky and the horizon. This causes aliasing inherent to the measurement itself and is purely a consequence of the Fourier basis.
N. Barry   +4 more
doaj   +1 more source

Improved Limits on the 21 cm Signal at z = 6.5–7.0 with the Murchison Widefield Array Using Gaussian Information

open access: yesThe Astrophysical Journal
We explore the properties of interferometric data from high-redshift 21 cm measurements using the Murchison Widefield Array (MWA). These data contain the redshifted 21 cm signal, contamination from continuum foreground sources, and radiometric noise. The
Cathryn M. Trott   +31 more
doaj   +1 more source

The Galactic Disk North–South Asymmetry in Metallicity May Be a New Tracer for the Disk Warp

open access: yesThe Astrophysical Journal Letters
Galactic disk warp has been widely characterized by stellar distributions and stellar kinematics but has not been traced by stellar chemistry. Here, we use a sample with over 170,000 red clump (RC) stars selected from LAMOST and APOGEE first to establish
Weixiang Sun   +3 more
doaj   +1 more source

Limits on the 21 cm Power Spectrum at z = 6.5–7.0 from Murchison Widefield Array Observations

open access: yesThe Astrophysical Journal
This paper presents the spherically averaged 21 cm power spectrum derived from Epoch of Reionization (EoR) observations conducted with the Murchison Widefield Array (MWA). The analysis uses EoR0-field data, centered at (R.A. = 0 h , decl.
C. D. Nunhokee   +31 more
doaj   +1 more source

The Kinematic Signature of the Warp and Waves in the Milky Way Disk

open access: yesThe Astrophysical Journal
Using over 170,000 red clump (RC) stars selected from LAMOST and APOGEE, we conduct a detailed analysis of the stellar V _Z as a function of L _Z (or R _g ) across different ϕ bins for various disk populations.
Weixiang Sun   +3 more
doaj   +1 more source

The Age–Velocity Dispersion Relations of the Galactic Disk as Revealed by the LAMOST-Gaia Red Clump Stars

open access: yesThe Astrophysical Journal
Using nearly 230,000 red clump stars selected from LAMOST and Gaia, we conduct a comprehensive analysis of the stellar age–velocity dispersion relations (AVRs) for various disk populations, within 5.0 ≤ R ≤ 15.0 kpc and ∣ Z ∣ ≤ 3.0 kpc.
Weixiang Sun   +3 more
doaj   +1 more source

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