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Everything about Large Magellanic Cloud
Satellite galaxy of the Milky Way
The Large Magellanic Cloud (LMC) is a dwarf galaxy and satellite galaxy of the Milky Way. At a distance of around 50 kiloparsecs, the LMC is the second- or third-closest galaxy to the Milky Way, after the Sagittarius Dwarf Spheroidal and the possible dwarf irregular galaxy called the Canis Major Overdensity. It is about 9.86 kiloparsecs across and has roughly one-hundredth the mass of the Milky Way, making it the fourth-largest galaxy in the Local Group after the Andromeda Galaxy (M31), the Milky Way, and the Triangulum Galaxy (M33). Wikipedia →
🧭 Start here: a 6-step reading path
- Read the overview: Large Magellanic CloudA 5-minute orientation
- Skim a recent paper: The Effect of the LMC on the Milky Way SystemInfluential work since 2022
- Pick up a classic book: Reflective Cracking in PavementsThe most-reprinted book on the subject
- Read the landmark paper: LMC and galactic extinctionCited 344 times
- Go sideways: NGC 1866A closely related topic
- Go sideways: Small Magellanic CloudA closely related topic
📖 Definitions
Symbol ISO 639-3 language code for Limilngan.
🗂️ The subject at a glance
🏆 Landmark papers (most cited)
LMC and galactic extinction
Relative frequencies of Type Ia and Type II supernovae in the chemical evolution of the Galaxy, LMC and SMC
Detection of the neutrino signal from SN 1987A in the LMC using the INR Baksan underground scintillation telescope
A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)
Tango for three: Sagittarius, LMC, and the Milky Way
THE CONSTANT INNER-DISK RADIUS OF LMC X-3: A BASIS FOR MEASURING BLACK HOLE SPIN
Is the SMC Bound to the LMC? TheHubble Space TelescopeProper Motion of the SMC
Spectroscopy of giants in LMC clusters. I - Velocities, abundances, and the age-metallicity relation
🆕 Influential since 2022
The Effect of the LMC on the Milky Way System
The Recent LMC–SMC Collision: Timing and Impact Parameter Constraints from Comparison of Gaia LMC Disk Kinematics and N-body Simulations
The iron and oxygen content of LMC Classical Cepheids and its implications for the extragalactic distance scale and Hubble constant
A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models
The VMC survey – XLVIII. Classical cepheids unveil the 3D geometry of the LMC
📚 Books worth reading
Reflective Cracking in PavementsJ. M. Rigo · 1993- 📕Descendants of Roderick and Christiana CameronL. Marilyn Cameron Stinson · 2007
- 📕LMC scheme of delegationWarwickshire (England). Education Department. · 1990
- 📕LMC Cleaning Services LLCGiorgio Armani · 2015
- 📕LMC selected areasMati Morel · 1990
- 📕LMC annual report.
- 📕LMC beef & sheep yearbookLivestock and Meat Commission for Northern Ireland. · 2003
- 📕Leucémies Myéloïdes Chroniques (LMC)Isaac ZOFFOUN · 2021
Ranked by number of editions on Open Library, a rough measure of how lasting a book is.
🔗 Related topics
- NGC 1866 NGC 1866 is a young globular cluster of stars near the northern edge of the Large Magellanic Cloud (LMC), located in the southern constellation of Dorado…
- Small Magellanic Cloud The Small Magellanic Cloud (SMC) is a dwarf galaxy near the Milky Way. Classified as a dwarf irregular galaxy, the SMC has a D25 isophotal diameter of…
- Tarantula Nebula The Tarantula Nebula (also known as 30 Doradus) is a large H II region in the Large Magellanic Cloud (LMC), forming its south-east corner (from Earth's…
- Cepheid variable A Cepheid variable (/ˈsɛfi.ɪd, ˈsiːfi-/) is a type of variable star that pulsates radially, varying in both diameter and temperature. It changes in brightness…
- NGC 5204 NCG 5204 is a Magellanic spiral galaxy located about 14.5 million light-years away from Earth in the constellation of Ursa Major and is a member of the…
- NGC 4449 NGC 4449, also known as Caldwell 21, is an irregular Magellanic type galaxy in the constellation Canes Venatici. It was discovered by German-British astronomer…
- NGC 1569 NGC 1569 is a dwarf irregular galaxy in Camelopardalis. The galaxy is relatively nearby, and consequently, the Hubble Space Telescope can easily resolve…
- Star cluster A star cluster is a group of stars, that share an origin, formed at roughly the same time and held together by self-gravitation. Two main types of star…