Results 91 to 100 of about 167,903 (283)
THE MAGELLANIC MOPRA ASSESSMENT (MAGMA). I. THE MOLECULAR CLOUD POPULATION OF THE LARGE MAGELLANIC CLOUD [PDF]
The Astrophysical Journal Supplement Series, 2011 We present the properties of an extensive sample of molecular clouds in the Large Magellanic Cloud (LMC) mapped at 11 pc resolution in the CO(1-0) line. We identify clouds as regions of connected CO emission, and find that the distributions of cloud sizes, fluxes and masses are sensitive to the choice of decomposition parameters. In all cases, however,
Wong, Tony +17 more
openaire +3 more sources
Lactea: Web‐Based Spectrum‐Preserving Multi‐Resolution Visualization of the GAIA Star Catalog
Computer Graphics Forum, Volume 44, Issue 3, June 2025.Abstract The explosion of data in astronomy has resulted in an era of unprecedented opportunities for discovery. The GAIA mission's catalog, containing a large number of light sources (mostly stars) with several parameters such as sky position and proper motion, is playing a significant role in advancing astronomy research and has been crucial in ...
Reem Alghamdi +3 more
wiley +1 more source
HIGH-AMPLITUDE δ-SCUTIS IN THE LARGE MAGELLANIC CLOUD [PDF]
The Astronomical Journal, 2010 26 pages, 15 figures, AJ ...
GARG A +15 more
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XMM‐Newton Observations of the Peculiar Be X‐Ray Binary A0538‐66
Astronomische Nachrichten, Volume 346, Issue 1, January 2025.ABSTRACT A0538‐66 is a neutron star/Be x‐ray binary located in the Large Magellanic Cloud and, since its discovery in the 70s, it showed a peculiar behavior that makes it a unique object in the high‐mass x‐ray binaries scene: the extremely eccentric orbit (e=0.72$$ e=0.72 $$), the short spin period of the neutron star (P=69$$ P=69 $$ ms), the episodes ...
Michela Rigoselli +3 more
wiley +1 more source
Molecular Cloud Structure in the Magellanic Clouds: Effect of Metallicity [PDF]
, 1997 The chemical structure of neutral clouds in low metallicity environments is examined with particular emphasis on the H to H_2 and C+ to CO transitions.
Booth, R.S. (Chalmers Tekniska Hoegskola, Goeteborg (Sweden). Raaoe Rymdobservatorium) +6 more
core +2 more sources
Large Magellanic Cloud Near-infrared Synoptic Survey. V. Period–Luminosity Relations of Miras [PDF]
, 2017 We study the near-infrared properties of 690 Mira candidates in the central region of the Large Magellanic Cloud, based on time-series observations at JHKs.
W. Yuan +5 more
semanticscholar +1 more source
The Large Magellanic Cloud: Structure and kinematics [PDF]
, 2006 Invited Review, 25 pages with 10 figures, to appear in "The Local Group as an Astrophysical Laboratory", Proceedings of the May 2003 STScI Symposium, M. Livio, ed., Cambridge, UK: Cambridge University Press. PDF file with higher-resolution figures available at http://www.stsci.edu/~marel/pdfdir/LMC_maysymp03_vdm3 ...
openaire +2 more sources
Structure of the Large Magellanic Cloud from 2MASS [PDF]
The Astrophysical Journal, 2001 This is a pre-published version which is collected from arXiv link.
Weinberg, MD, Nikolaev, S
openaire +3 more sources
Beyond Accretion Limits: The Rise of Pulsating Gems
Astronomische Nachrichten, Volume 346, Issue 1, January 2025.ABSTRACT The discovery of several ultraluminous X‐ray sources exhibiting fast and rapidly evolving X‐ray pulsations unequivocally associates these sources with accreting neutron stars orbiting relatively massive companion stars (> 8M ⊙$$ {}_{\odot } $$).
Gian Luca Israel +26 more
wiley +1 more source
Five Massive Contact Binaries with Twin Components in LMC
The Astrophysical Journal, 2023 Massive contact binaries refer to the close binary systems in which the components have filled their respective Roche lobes and share a common envelope with early-type spectra.
Fu-Xing Li +8 more
doaj +1 more source