ERD

Periodic Reporting for period 3 - MULTIPLES (The MULTIPLicity of supErnova progenitorS)

Project: MULTIPLES

Updated at: 01-11-2024

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Project acronym MULTIPLES

The First Dynamical Mass Determination of a Nitrogen-rich Wolf–Rayet Star Using a Combined Visual and Spectroscopic Or...

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Modeling contact binaries II. Effects of energy transfer

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars: II. The northern WNE sequence

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

The Carina High-contrast Imaging Project for massive Stars (CHIPS): II. O stars in Trumpler~14

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

The Tarantula Massive Binary Monitoring

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

The Galactic WC and WO stars

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Multiplicity of the red supergiant population in the young massive cluster NGC 330

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Clues on the Origin and Evolution of Massive Contact Binaries: Atmosphere Analysis of VFTS 352

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

The stellar and wind parameters of six prototypical HMXBs and their evolutionary status

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Testing massive star evolution, star formation history, and feedback at low metallicity

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

The VLT-FLAMES Tarantula Survey

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Why binary interaction does not necessarily dominate the formation of Wolf-Rayet stars at low metallicity

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Low-metallicity massive single stars with rotation

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

On the signature of a 70-solar-mass black hole in LB-1

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Uncovering astrometric black hole binaries with massive main-sequence companions with Gaia

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

(Sub)stellar companions shape the winds of evolved stars

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Constraining the overcontact phase in massive binary evolution

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC 346 in th...

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

The Wolf–Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Is HR 6819 a triple system containing a black hole?

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Detailed models of interacting short-period massive binary stars

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

The Galactic WN stars revisited

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

The Tarantula Massive Binary Monitoring III. Atmosphere analysis of double-lined spectroscopic systems

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Modeling overcontact binaries, I. The effect of tidal deformation

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Detailed evolutionary models of massive contact binaries – I. Model grids and synthetic populations for the Magellanic...

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Tying the Geometrical Traits of Massive Young Stellar Objects and Their Disks to a Potential Evolutionary Sequence Using...

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

The young massive SMC cluster NGC 330 seen by MUSE

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

https://arxiv.org/abs/2205.11318

Project: MULTIPLES

Updated at: 27-04-2024

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Project acronym MULTIPLES

Resources

Selected filters:

Periodic Reporting for period 3 - MULTIPLES (The MULTIPLicity of supErnova progenitorS)

The First Dynamical Mass Determination of a Nitrogen-rich Wolf–Rayet Star Using a Combined Visual and Spectroscopic Or...

Modeling contact binaries II. Effects of energy transfer

A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars: II. The northern WNE sequence

The Carina High-contrast Imaging Project for massive Stars (CHIPS): II. O stars in Trumpler~14

The Tarantula Massive Binary Monitoring

The Galactic WC and WO stars

Multiplicity of the red supergiant population in the young massive cluster NGC 330

Clues on the Origin and Evolution of Massive Contact Binaries: Atmosphere Analysis of VFTS 352

The stellar and wind parameters of six prototypical HMXBs and their evolutionary status

Testing massive star evolution, star formation history, and feedback at low metallicity

The VLT-FLAMES Tarantula Survey

Why binary interaction does not necessarily dominate the formation of Wolf-Rayet stars at low metallicity

Low-metallicity massive single stars with rotation

On the signature of a 70-solar-mass black hole in LB-1

A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars

Uncovering astrometric black hole binaries with massive main-sequence companions with Gaia

(Sub)stellar companions shape the winds of evolved stars

Constraining the overcontact phase in massive binary evolution

Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC 346 in th...

The Wolf–Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud

Is HR 6819 a triple system containing a black hole?

Detailed models of interacting short-period massive binary stars

The Galactic WN stars revisited

The Tarantula Massive Binary Monitoring III. Atmosphere analysis of double-lined spectroscopic systems

Modeling overcontact binaries, I. The effect of tidal deformation

Detailed evolutionary models of massive contact binaries – I. Model grids and synthetic populations for the Magellanic...

Tying the Geometrical Traits of Massive Young Stellar Objects and Their Disks to a Potential Evolutionary Sequence Using...

The young massive SMC cluster NGC 330 seen by MUSE

https://arxiv.org/abs/2205.11318