Results 51 to 60 of about 29,911 (101)

Rutting and rambling: Movement characteristics reveal partial migration in adult male white‐tailed deer at a latitude void of chronic and severe environmental fluctuations

open access: yesEcology and Evolution, Volume 14, Issue 2, February 2024.
Some white‐tailed deer populations are migratory in locations with severe and chronic seasonal resource limitations, but biological justification for such behaviors is lacking at lower latitudes. We document migratory behavior termed the "mobile" movement strategy in 33% of adult male deer in a low‐latitude system void of such environmental pressures ...
Luke Resop   +4 more
wiley   +1 more source

In Pursuit of the Least Luminous Galaxies

open access: yesAdvances in Astronomy, Volume 2010, Issue 1, 2010., 2010
The dwarf galaxy companions to the Milky Way are unique cosmological laboratories. With luminosities as low as 10−7LMW, they inhabit the lowest mass dark matter halos known to host stars and are presently the most direct tracers of the distribution, mass spectrum, and clustering scale of dark matter.
Beth Willman, Regina Schulte-Ladbeck
wiley   +1 more source

The Truncated Circumgalactic Medium of the Large Magellanic Cloud

open access: yesThe Astrophysical Journal Letters
The Large Magellanic Cloud (LMC) is the nearest massive galaxy to the Milky Way (MW). Its circumgalactic medium (CGM) is complex and multiphase, containing both stripped H i structures like the Magellanic Stream and Bridge and a diffuse warm corona seen ...
Sapna Mishra   +8 more
doaj   +1 more source

The Relevance of Dynamical Friction for the MW/LMC/SMC Triple System

open access: yesUniverse
Simulations of structure formation in the standard cold dark matter cosmological model quantify the dark matter halos of galaxies. Taking into account dynamical friction between dark matter halos, we investigate the past orbital dynamical evolution of ...
Wolfgang Oehm, Pavel Kroupa
doaj   +1 more source

Monitoring of X‐Ray Sources in the Optical Spectral Region

open access: yesAdvances in Astronomy, Volume 2010, Issue 1, 2010., 2010
We review current results and perspectives of the photometric monitoring of the optical counterparts of X‐ray sources of various kinds (binary X‐ray sources (cataclysmic variables and low‐mass X‐ray binaries, supersoft X‐ray sources, microquasars), gamma‐ray bursts).
Vojtěch Šimon, Lorraine Hanlon
wiley   +1 more source

The Metallicities of Five Small High-velocity Clouds

open access: yesThe Astrophysical Journal
High-velocity clouds (HVCs) are multiphase gas structures whose velocities (∣ v _LSR ∣ ≥ 100 km s ^−1 ) are too high to be explained by Galactic disk rotation.
Trisha Ashley   +7 more
doaj   +1 more source

The detection of an older population in the Magellanic Bridge [PDF]

open access: yes, 2012
The Magellanic system comprises the Large Magellanic Cloud (LMC), the Small Magellanic Cloud (SMC), and the less frequently observed Magellanic Bridge and Magellanic Stream. The Bridge is traced by neutral gas and has an observed stellar component, while the Stream consists of gas only, with no observed stellar counterpart to date.
arxiv   +1 more source

The Multiple Extended Tidal Tails of NGC 288

open access: yesThe Astrophysical Journal
Using photometry and proper motions from Pan-STARRS, DECaLS, and Gaia Data Release 3, we detect a ∼35°–70° long trailing stellar debris stream associated with the globular cluster NGC 288.
Carl J. Grillmair
doaj   +1 more source

A Neutral Hydrogen Absorption Study of Cold Gas in the Outskirts of the Magellanic Clouds Using the GASKAP-H i Survey

open access: yesThe Astronomical Journal
Cold neutral hydrogen (H i ) is a crucial precursor for molecular gas formation and can be studied via H i absorption. This study investigates H i absorption in low column density regions of the Small and Large Magellanic Clouds (SMC and LMC) using the ...
Hongxing Chen   +20 more
doaj   +1 more source

Revealing the Ionization Properties of the Magellanic Stream using Optical Emission [PDF]

open access: yes, 2017
The Magellanic Stream, a gaseous tail that trails behind the Magellanic Clouds, could replenish the Milky Way with a tremendous amount of gas if it reaches the Galactic disk before it evaporates into the halo. To determine how the Magellanic Stream's properties change along its length, we have conducted an observational study of the H-alpha emission ...
arxiv   +1 more source

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