Results 151 to 160 of about 167,903 (283)

INTEGRAL observations of the Large Magellanic Cloud region

, 2004
We present the preliminary results of the INTEGRAL survey of the Large Magellanic Cloud. The observations have been carried out in January 2003 (about 10^6 s) and January 2004 (about 4x10^5 s).
Belloni, T., Courvoisier, T., Dean, A., Ebisawa, K., Gotz, D., Hakala, P., Knodlseder, J., Kretschmar, P., Mereghetti, S., Paizis, A., Pellizzoni, A., Stella, L., Strong, A., Swings, J. -P., Vercellone, S., Vilhu, O., Walter, R., Westergaard, N. J., Zdziarski, A.   +18 more
core  

Large-scale structure and kinematics of the Magellanic Clouds from carbon star studies [PDF]

, 1991
M. Azzopardi, E. Rebeirot
openalex   +1 more source

LMC-driven Anisotropic Boosts in Stream–Subhalo Interactions

The Astrophysical Journal
Dark matter subhalos are predicted to perturb stellar streams; stream morphologies and dynamics can, therefore, constrain the mass distribution of subhalos.
Arpit Arora, Nicolás Garavito-Camargo, Robyn E. Sanderson, Emily C. Cunningham, Andrew Wetzel, Nondh Panithanpaisal, Megan Barry   +6 more
doaj   +1 more source

A New and Unusual Variable Star in the Large Magellanic Cloud [PDF]

, 1969
Frances W. Wright, P. W. Hodge
openalex   +1 more source

The Detection of Higher-order Millimeter Hydrogen Recombination Lines in the Large Magellanic Cloud [PDF]

, 2023
M. Sewiło, Kazuki Tokuda, S. Kurtz, Steven B. Charnley, T. Möller, Jennifer Wiseman, C.‐H. Rosie Chen, R. Indebetouw, Á. Sánchez-Monge, Kei Tanaka, P. Schilke, Toshikazu Onishi, Naoto Harada   +12 more
openalex   +1 more source

NGC 1856: Using Machine Learning Techniques to Uncover Detailed Stellar Abundances from MUSE Data

The Astronomical Journal
We present the first application of the novel approach based on data-driven machine learning methods applied to Multi-Unit Spectroscopic Explorer (MUSE) field data to derive stellar abundances of star clusters.
Randa Asa’d, S. Hernandez, J. M John, M. Alfaro-Cuello, Z. Wang, A. As’ad, A. Vasini, F. Matteucci   +7 more
doaj   +1 more source

Response of the LMC’s Bar to a Recent SMC Collision and Implications for the SMC’s Dark Matter Profile

The Astrophysical Journal
The LMC’s stellar bar is offset from the outer disk center, tilted from the disk plane, and does not drive gas inflows. These properties are atypical of bars in gas-rich galaxies, yet the LMC bar’s strength and radius are similar to typical barred ...
Himansh Rathore, Gurtina Besla, Kathryne J. Daniel, Leandro Beraldo e Silva   +3 more
doaj   +1 more source

The MACHO Project Large Magellanic Cloud Variable Star Inventory. XII. Three Cepheid Variables in Eclipsing Binaries [PDF]

, 2002
C. Alcock, R. A. Allsman, D. R. Alves, A. C. Becker, D. P. Bennett, K. H. Cook, A. J. Drake, K. C. Freeman, K. Griest, Suzanne L. Hawley, S. Keller, M. J. Lehner, D. Lepischak, S. L. Marshall, D. Minniti, C. A. Nelson, B. A. Peterson, Piotr Popowski, M. R. Pratt, P. J. Quinn, A. W. Rodgers, N. B. Suntzeff, William J. Sutherland, T. Vandehei   +23 more
openalex   +1 more source

Erratum: “Kinematic Decomposition of the H i Gaseous Component in the Large Magellanic Cloud” (2022, ApJ, 928, 177) [PDF]

, 2023
Se–Heon Oh, Shinna Kim, Bi‐Qing For, L. Staveley‐Smith   +3 more
openalex   +1 more source

OGLE-IV Period–Luminosity Relation of the LMC: An Analysis Using Mean and Median Magnitudes

The Astronomical Journal
The Period–Luminosity (PL) relation for Cepheid variable stars in the LMC is crucial for distance measurements in astronomy. This study analyzes the impact of using the median rather than the mean of the PL relation’s slope and zero-point.
Jaime Muñoz, Alejandro García-Varela, Santiago Henao-Castellanos, Beatriz Sabogal, Luis Felipe Giraldo, Jorge Martínez   +5 more
doaj   +1 more source