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Toward Precision Measurement of Central Black Hole Masses

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Toward the End of Stars: Discovering the Galaxy's Coldest Brown Dwarfs

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Toward the Formation of Realistic Galaxy Disks

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Toward the general RGB slope-metallicity-age calibration: I Metallicities, Ages and Kinematics for Eight LMC Clusters

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Toward understanding the formation of multiple systems - A pilot IRAM-PdBI survey of Class 0 objects

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Towards a census of the Galactic anticentre star clusters II: exploring lower overdensities

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Towards a census of the Galactic anticentre star clusters: colour-magnitude diagram and structural analyses of a sample of 50 objects

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Towards a Complete Census of AGNs in Nearby Galaxies: The Incidence of Growing Black Holes

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Towards a fully consistent Milky Way disc model - II. The local disc model and SDSS data of the NGP region

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Towards a fully consistent Milky Way disc model: Part 1 The local model based on kinematic and photometric data

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Towards a library of synthetic galaxy spectra and preliminary results of classification and parametrization of unresolved galaxies for Gaia - II

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Towards a new full-sky list of radial velocity standard stars

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Towards a precise measurement of the cosmic-ray positron fraction

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Towards a self-consistent numerical model of late-type galaxies: Calibrating the effects of sub-grid physics on galactic models

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Towards constraining the central black hole's properties by studying its infrared flares with the GRAVITY instrument

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Towards relativistic orbit fitting of Galactic center stars and pulsars

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Towards understanding the dynamics of the bar/bulge region in our Galaxy

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Tracing early evolutionary stages of high-mass star formation with molecular lines

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Tracing gas accretion in the Galactic center using isotopic ratios

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Tracing Magnetic Fields with Ground State Alignment

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