The VMC survey – XLI. Stellar proper motions within the Small Magellanic Cloud [PDF]
We used data from the near-infrared Visible and Infrared Telescope for Astronomy (VISTA) survey of the Magellanic Cloud system (VMC) to measure proper motions (PMs) of stars within the Small Magellanic Cloud (SMC).
F. Niederhofer +15 more
semanticscholar +1 more source
A Distance Determination to the Small Magellanic Cloud with an Accuracy of Better than Two Percent Based on Late-type Eclipsing Binary Stars [PDF]
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
ALMA Reveals a Cloud–Cloud Collision that Triggers Star Formation in the Small Magellanic Cloud [PDF]
We present the results of Atacama Large Millimeter/submillimeter Array observations in 12CO(1–0) emission at 0.58 × 0.52 pc2 resolution toward the brightest H ii region N66 of the Small Magellanic Cloud (SMC).
Naslim Neelamkodan +5 more
semanticscholar +1 more source
Discovery of the Magellanic Stellar Stream Out to 100 kpc
The Magellanic Stream (MS)—an enormous ribbon of gas spanning 140° of the southern sky trailing the Magellanic Clouds—has been exquisitely mapped in the five decades since its discovery.
Vedant Chandra +9 more
doaj +1 more source
Magellanic Clouds Cepheids: Thorium Abundances [PDF]
The analysis of the high-resolution spectra of 31 Magellanic Clouds Cepheid variables enabled the identification of thorium lines. The abundances of thorium were found with spectrum synthesis method. The calculated thorium abundances exhibit correlations
Yeuncheol Jeong +5 more
doaj +1 more source
Optical spectra of radio planetary nebulae in the large Magellanic Cloud [PDF]
We present 11 spectra from 12 candidate radio sources co-identified with known planetary nebulae (PNe) in the Large Magellanic Cloud (LMC). Originally found in Australia Telescope Compact Array (ATCA) LMC surveys at 1.4, 4.8 and 8.64 GHz and confirmed by
Payne J.L. +6 more
doaj +3 more sources
Runaway OB Stars in the Small Magellanic Cloud: Dynamical versus Supernova Ejections [PDF]
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
CCD imagers for the Transiting Exoplanet Survey Satellite from benchtop to space environment
Abstract The Transiting Exoplanet Survey Satellite (TESS) is a Massachusetts Institute of Technology‐led NASA Explorer‐class mission planned to spend 2 years discovering transiting exoplanets by an all‐sky survey. The observatory contains four wide field‐of‐view camera systems for a total of 16.8 Megapixel, low‐noise, low‐power CCD detectors.
Vyshnavi Suntharalingam +5 more
wiley +1 more source
The nature of molecular clouds and their statistical behavior in subsolar metallicity environments are not fully explored yet. We analyzed data from an unbiased CO ( J = 2–1) survey at the spatial resolution of ∼2 pc in the northern region of the Small ...
Takahiro Ohno +18 more
doaj +1 more source
LRO‐LAMP Lunar South Pole Cold Traps: Assessment of H2O and Potential CO2 and NH3 Reserves
Abstract Nighttime Lyman Alpha Mapping Project (LAMP) observations are used to investigate condensed volatiles at the south polar region of the Moon. This study incorporates LAMP data from the first ∼7 years of the mission and Diviner annual maximum temperatures to search for volatile signatures associated with H2O, NH3, and CO2. Other stable potential
L. O. Magaña +15 more
wiley +1 more source

