Results 21 to 30 of about 343,655 (292)

X-ray Pulsars in the Small Magellanic Cloud [PDF]

open access: yesThe Astrophysical Journal, 2004
XMM-Newton archival data for the Small Magellanic Cloud have been examined for the presence of previously undetected X-ray pulsars. One such pulsar, with a period of 202 s, is detected.
Corbet R.   +11 more
core   +5 more sources

The 3D Kinematics of Gas in the Small Magellanic Cloud [PDF]

open access: yesThe Astrophysical Journal, 2019
We investigate the kinematics of neutral gas in the Small Magellanic Cloud (SMC) and test the hypothesis that it is rotating in a disk. To trace the 3D motions of the neutral gas distribution, we identify a sample of young, massive stars embedded within ...
C. Murray   +5 more
semanticscholar   +6 more sources

The Magellanic Squall: Gas Replenishment from the Small to Large Magellanic Cloud [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2007
We first show that a large amount of metal-poor gas is stripped from the Small Magellanic Cloud (SMC) and fallen into the Large Magellanic Cloud (LMC) during the tidal interaction between the SMC, the LMC, and the Galaxy over the last 2 Gyrs.
Bekki, Kenji, Chiba, Masashi
core   +4 more sources

The Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE): The Dust Extinction Curve from Red Clump Stars [PDF]

open access: yes, 2017
We use Hubble Space Telescope (HST) observations of red clump stars taken as part of the Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE) program to measure the average dust extinction curve in a ∼200 pc × 100 pc region in the ...
Petia Yanchulova Merica-Jones   +9 more
semanticscholar   +5 more sources

Velocity and Density Spectra of the Small Magellanic Cloud [PDF]

open access: greenThe Astrophysical Journal, 2001
5 pages, 1 figure, accepted for publication in the ApJ ...
Snežana Stanimirović, A. Lazarian
openalex   +4 more sources

The Phanerozoic climate. [PDF]

open access: yesAnn N Y Acad Sci, 2023
We review the long‐term climate variations during the last 540 million years (Phanerozoic Eon). We first summarize the geological and geochemical datasets available for reconstruction of long‐term climate variations. We then explore the main drivers of climate that appear to explain a large fraction of these climatic oscillations. The first is the long‐
Shaviv NJ, Svensmark H, Veizer J.
europepmc   +2 more sources

A Distance Determination to the Small Magellanic Cloud with an Accuracy of Better than Two Percent Based on Late-type Eclipsing Binary Stars [PDF]

open access: yesAstrophysical Journal, 2020
We present a new study of late-type eclipsing binary stars in the Small Magellanic Cloud (SMC) undertaken with the aim of improving the distance determination to this important galaxy.
D. Graczyk   +19 more
semanticscholar   +1 more source

Understanding climate change impacts on biome and plant distributions in the Andes: Challenges and opportunities. [PDF]

open access: yesJ Biogeogr, 2022
Abstract Aim Climate change is expected to impact mountain biodiversity by shifting species ranges and the biomes they shape. The extent and regional variation in these impacts are still poorly understood, particularly in the highly biodiverse Andes. Regional syntheses of climate change impacts on vegetation are pivotal to identify and guide research ...
Tovar C   +24 more
europepmc   +2 more sources

Improved Campephiline detection: An experiment conducted with the Magellanic Woodpecker. [PDF]

open access: yesEcol Evol, 2019
We designed an experiment to determine which of three methods best results in a detection of Magellanic Woodpeckers (Campephilus magellanicus). The drumming device most effectively influenced the likelihood of a woodpecker detection. Using a drumming device likely will be an effective technique to detect not only Magellanic Woodpeckers, but other ...
Wynia AL, Rolland V, Jiménez JE.
europepmc   +2 more sources

Runaway OB Stars in the Small Magellanic Cloud: Dynamical versus Supernova Ejections [PDF]

open access: yesAstrophysical Journal, 2020
Runaway OB stars are ejected from their parent clusters via two mechanisms, both involving multiple stars: the dynamical ejection scenario (DES) and the binary supernova scenario (BSS).
J. Jones   +4 more
semanticscholar   +1 more source

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