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The Luminosity Functions and Timescales of MYSOs and Compact HII regions

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The Luminosity, Mass, and Age Distributions of Compact Star Clusters in M83 Based on HST/WFC3 Observations

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter

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The MACHO Project HST Follow-Up: The Large Magellanic Cloud Microlensing Source Stars

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The Magellanic Mopra Assessment (MAGMA). I. The Molecular Cloud Population of the Large Magellanic Cloud

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The Magellanic Stream to Halo Interface: Processes that shape our nearest gaseous Halo Stream

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The magnetar origin of pulsars

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The Magnetic Field in Taurus Probed by Infrared Polarization

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The magnetic field in the NGC 2024 FIR 5 dense core

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The magnetic field of IRAS 16293-2422 as traced by shock-induced H2O masers

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The Magnetic Field of the H~II Region NGC 6334A

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The Magnetic Field of the Irregular Galaxy NGC 4214

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The Magnetic Field of the Milky Way Galaxy

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The Magnetized Environment of the W3(H2O) Protostars

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The magneto-ionic medium in the Milky Way

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The Masers Towards IRAS 20126+4104

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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The Mass and Radius of the Neutron Star in the Bulge Low-Mass X-ray Binary KS 1731-260

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The mass and velocity anisotropy of the Carina, Fornax, Sculptor and Sextans dwarf spheroidal galaxies

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The Mass Distribution and Assembly of the Milky Way from the Properties of the Magellanic Clouds

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The Mass Distribution of Stellar-Mass Black Holes

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