Laboratoire d'Astrophysique de Bordeaux (LAB)

Le Laboratoire d’astrophysique de Bordeaux (LAB) est une unité mixte de recherche (UMR) entre l’Université de Bordeaux (UB) et le Centre national de la recherche scientifique (CNRS). C’est l’une des unités constitutives de l’Observatoire aquitain des sciences de l’Univers (OASU), lui-même à la fois école interne du Département Sciences et Technologies de l’UB et observatoire des sciences de l’Univers (OSU) de l’Institut national des sciences de l’Univers (INSU) du CNRS. Le LAB remplit trois missions principales : la recherche fondamentale en sciences de l’Univers, la formation des étudiants par la recherche, la diffusion de la culture scientifique et technique.

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Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804

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Recent Submissions

Predicting HCN, HCO<SUP>+</SUP>, multi-transition CO, and dust emission of star-forming galaxies. Constraining the properties of resolved gas and dust disks of local spiral galaxies

Characterizing the astrometric instability of extragalactic radio source positions measured with geodetic VLBI

SiS Formation in the Interstellar Medium through Si+SH Gas-phase Reactions

SF2A-2021: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics.

Reaction N( 2 D) + CH 2 CCH 2 (Allene): An Experimental and Theoretical Investigation and Implications for the Photochemical Models of Titan

GLOSTAR -- Radio Source Catalog II: $28^\circ < \ell < 36^\circ$ and $|b| < 1^\circ$, VLA B-configuration

Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds

Sulphur-rich cold gas around the hot core precursor G328.2551-0.5321

The SEDIGISM survey: Molecular cloud morphology

ALMA-IMF. IV. A comparative study of the main hot cores in W43-MM1: Detection, temperature, and molecular composition

The SEDIGISM survey: A search for molecular outflows

The evolution of temperature and density structures of OB cluster-forming molecular clumps

Disk fragmentation in high-mass star formation

Combination at the Observation Level:contribution to ITRF2013

Combination at the Observation Level: contribution to ITRF2013

Molecular and ionized gas in the tidal tail in Stephan's Quintet

PRODIGE - Envelope to disk with NOEMA

Chemical Richness of protoplanetary Disks and related physical Properties

Kelvin-Helmholtz instability and induced magnetic reconnection at the Earth’s magnetopause: a 3D simulation based on satellite data

Disentangling the main populations of the Zodiacal Cloud from Zodiacal Light observations

Statistics

Collection General Statistics

Typology History

Recent submissions distribution

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804

Browse by

Recent Submissions

Predicting HCN, HCO<SUP>+</SUP>, multi-transition CO, and dust emission of star-forming galaxies. Constraining the properties of resolved gas and dust disks of local spiral galaxies ﻿

Characterizing the astrometric instability of extragalactic radio source positions measured with geodetic VLBI ﻿

SiS Formation in the Interstellar Medium through Si+SH Gas-phase Reactions ﻿

SF2A-2021: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. ﻿

Reaction N( 2 D) + CH 2 CCH 2 (Allene): An Experimental and Theoretical Investigation and Implications for the Photochemical Models of Titan ﻿

GLOSTAR -- Radio Source Catalog II: $28^\circ < \ell < 36^\circ$ and $|b| < 1^\circ$, VLA B-configuration ﻿

Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds ﻿

Sulphur-rich cold gas around the hot core precursor G328.2551-0.5321 ﻿

The SEDIGISM survey: Molecular cloud morphology ﻿

ALMA-IMF. IV. A comparative study of the main hot cores in W43-MM1: Detection, temperature, and molecular composition ﻿

The SEDIGISM survey: A search for molecular outflows ﻿

The evolution of temperature and density structures of OB cluster-forming molecular clumps ﻿

Disk fragmentation in high-mass star formation ﻿

Combination at the Observation Level:contribution to ITRF2013 ﻿

Combination at the Observation Level: contribution to ITRF2013 ﻿

Molecular and ionized gas in the tidal tail in Stephan's Quintet ﻿

PRODIGE - Envelope to disk with NOEMA ﻿

Chemical Richness of protoplanetary Disks and related physical Properties ﻿

Kelvin-Helmholtz instability and induced magnetic reconnection at the Earth’s magnetopause: a 3D simulation based on satellite data ﻿

Disentangling the main populations of the Zodiacal Cloud from Zodiacal Light observations ﻿

Statistics

Collection General Statistics

Typology History

Recent submissions distribution

Predicting HCN, HCO<SUP>+</SUP>, multi-transition CO, and dust emission of star-forming galaxies. Constraining the properties of resolved gas and dust disks of local spiral galaxies

Characterizing the astrometric instability of extragalactic radio source positions measured with geodetic VLBI

SiS Formation in the Interstellar Medium through Si+SH Gas-phase Reactions

SF2A-2021: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics.

Reaction N( 2 D) + CH 2 CCH 2 (Allene): An Experimental and Theoretical Investigation and Implications for the Photochemical Models of Titan

GLOSTAR -- Radio Source Catalog II: $28^\circ < \ell < 36^\circ$ and $|b| < 1^\circ$, VLA B-configuration

Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds

Sulphur-rich cold gas around the hot core precursor G328.2551-0.5321

The SEDIGISM survey: Molecular cloud morphology

ALMA-IMF. IV. A comparative study of the main hot cores in W43-MM1: Detection, temperature, and molecular composition

The SEDIGISM survey: A search for molecular outflows

The evolution of temperature and density structures of OB cluster-forming molecular clumps

Disk fragmentation in high-mass star formation

Combination at the Observation Level:contribution to ITRF2013

Combination at the Observation Level: contribution to ITRF2013

Molecular and ionized gas in the tidal tail in Stephan's Quintet

PRODIGE - Envelope to disk with NOEMA

Chemical Richness of protoplanetary Disks and related physical Properties

Kelvin-Helmholtz instability and induced magnetic reconnection at the Earth’s magnetopause: a 3D simulation based on satellite data

Disentangling the main populations of the Zodiacal Cloud from Zodiacal Light observations