Results 111 to 120 of about 104,909 (264)
Mass Spectrometry Reviews, Volume 44, Issue 3, Page 213-453, May/June 2025.Abstract The use of matrix‐assisted laser desorption/ionization (MALDI) mass spectrometry for the analysis of carbohydrates and glycoconjugates is a well‐established technique and this review is the 12th update of the original article published in 1999 and brings coverage of the literature to the end of 2022.
David J. Harvey
wiley +1 more source
The Chemical Evolution of the Milky Way Galaxy
, 2021 The elemental abundance gradients of elements up to Zn are predicted using the N body Monte Carlo technique by developing homogenous and heterogeneous Galactic Chemical Evolution (GCE) simulations. In the case of homogeneous GCE models, the galaxy is radially divided into eight annular rings of 2 kpc width each at a distance of 2-18 kpc from the center
openaire +2 more sources
Metallicity Mapping of the Ionized Diffuse Gas at the Milky Way Disk–Halo Interface
The Astrophysical JournalMetals in the diffuse, ionized gas at the boundary between the Milky Way’s interstellar medium (ISM) and circumgalactic medium, known as the disk–halo interface (DHI), are valuable tracers of the feedback processes that drive the Galactic fountain ...
Bo-Eun Choi +7 more
doaj +1 more source
Global warming and obesity: External heat exposure as a modulator of energy balance
FASEB BioAdvances, Volume 7, Issue 4, April 2025.Core body temperature regulation can significantly influence metabolic processes to maintain energy balance. For example, geographic and environmental factors (global warming) can affect obesity rates and can be tracked along latitudinal boundaries.
Imani Muhammad +3 more
wiley +1 more source
A catalog of galaxies behind the Southern Milky Way [PDF]
, 2000 R. C. Kraan‐Korteweg
openalex +2 more sources
Rotation and mass in the Milky Way and spiral galaxies [PDF]
Publications of the Astronomical Society of Japan, 2016 Abstract Rotation curves are the basic tool for deriving the distribution of mass in spiral galaxies. In this review, we describe various methods to measure rotation curves in the Milky Way and spiral galaxies. We then describe two major methods to calculate the mass distribution using the rotation curve.
openaire +4 more sources
, 2012 Our 'home galaxy' - the Milky Way - is a fairly large spiral galaxy, prototype of the most common morphological class in the local Universe. Although being only a galaxy, it is the only one that can be studied in unique detail: for the MilkyWay and for a
De Lucia, Gabriella
core +1 more source
The Astrophysical JournalUnderstanding the physical mechanism behind the formation of a corotating thin plane of satellite galaxies, like the one observed around the Milky Way (MW), has been challenging.
Nicolás Garavito-Camargo +10 more
doaj +1 more source
Impact of the low solar abundance on the ages of globular clusters
, 2010 We present the result of our investigation on the impact of the low Solar abundance of Asplund and collaborators (2004) on the derived ages for the oldest star clusters based on isochrone fittings. We have constructed new stellar models and corresponding
Kim, Yong -Cheol, Yi, Sukyoung K.
core +1 more source
The Astrophysical JournalThe Milky Way (MW) is a barred spiral galaxy shaped by tidal interactions with its satellites. The Large Magellanic Cloud (LMC) and the Sagittarius dwarf galaxy (Sgr) are the dominant influences at the present day. This paper presents a suite of four 10 ^
Ioana A. Stelea +2 more
doaj +1 more source