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Combining Planck and Herschel to improve our view of the Milky Way | ||
Observed properties of interstellar filaments: Insights into the initial conditions for star formation | ||
The Forgotten Quadrant Survey: A high-quality 12CO/13CO survey of the 3rd Milky Way Quadrant | ||
Deuterated methanol map towards L1544 | ||
Fragmenting filaments in simulations | ||
Nitrogen fractionation in high-mass star forming cores and its Galactic trend | ||
Determining the initial gas structure in cold, massive clumps: Cluster formation in its earliest stages | ||
Non-thermal states in models of filaments: A dynamical study | ||
The ATLASGAL Survey: Evolution of high-mass star-forming regions | ||
Towards a physically motivated core definition: The Pipe Nebula as seen in Herschel-Planck emission and NIR extinction | ||
A Kennicutt-Schmidt relation at molecular cloud scales and beyond | ||
Time evolution of giant molecular cloud mass functions with cloud-cloud collisions and gas resurrection in various environments | ||
OMC-2 FIR 4: A laboratory to study the formation environment of the Solar System | ||
How does early stellar feedback alter the impact of later supernovae? | ||
Multiple star formation of a starless core being part of a filament in the Orion A cloud | ||
Star formation and ionized regions throughout the inner Galactic plane | ||
SOFIA science highlights of star formation studies | ||
Tracing star formation with non-thermal radio emission | ||
Polytropic models of filamentary molecular clouds | ||
Galactic fountain flows in high resolution hydrodynamical simulations of galaxy discs | ||
ALMA view of the massive dense core in the Galactic center 50km/s molecular cloud | ||
The ionized gas in the Milky Way as seen with THOR | ||
A ram-pressure threshold for star formation | ||
Gravity drives the evolution of infrared dark hubs | ||
Investigation of star formation activities in the Galactic giant filaments | ||
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Mid-infrared interferometric variability of DG Tau: implications for the inner disk structure? | ||
Grain growth in Class I protostar Per-emb-50: A dust continuum analysis with NOEMA & SMA | ||
Disk kinematics in high-mass star formation | ||
Unveiling YSO dynamics through observations and simulations | ||
Chemical modeling of small scale chemical segregation | ||
On the dynamical feedback of asymmetric jets on protoplanetary disks | ||
First submillimeter detection of the disk around a young, isolated, planetary-mass object | ||
How organics deuteration changes during the formation of a Sun-like star | ||
Spectro-astrometric study of the Halpha emission of the T Tauri star T Cha to detect any contribution from its substellar companion T Cha b | ||
First disk-mediated accretion burst from a massive protostar | ||
The near-ultraviolet as the true window on jet rotation | ||
Eruptive variable protostars from VVV | ||
Investigating accretion-ejection with optical interferometry | ||
Radiative feedback and thresholds for massive star formation: theory and numerical simulations | ||
Physical properties of the cold cores in Serpens | ||
A 1000 AU scale molecular outflow driven by a candidate first hydrostatic core in a filament supported by MHD turbulence | ||
Massive star formation by accretion: How to circumvent the angular momentum barrier? | ||
Protostellar outflows in different star-forming environments | ||
First light emerging from the clouds | ||
Line-driven ablation of star forming disks | ||
Fantastic YSOs and photoevaporating protoplanetary disks in the Orion’s sibling - NGC 1977 | ||
From accretion to outflows of massive protostars | ||
ALMA observations of the envelope-to-disk mass transport in the FU Orionis-type young eruptive star V346 Normae | ||
Revisiting the pre-main sequence evolution of stars: Importance of accretion efficiency and deuterium abundance | ||
Binary star formation and the outflows from their discs | ||
A Keplerian rotating accretion disk and a spinning jet in the HH 212 protostellar system | ||
Synthetic observations of core fragmentation and young multiples | ||
Connection between the accretion and outflow processes in T Tauri stars | ||
Measuring the H2O snowline in protoplanetary disks | ||
Massive outflow driven by magnetic effects with high mass accretion rates | ||
Spectroscopy of 400-1000 au companions to dusty Orion young stellar objects | ||
Evolutionary indicators in dense clumps from the Hi-GAL survey | ||
The impact of large-scale flows in high-mass star forming regions | ||
Properties of a jet from the T Tauri star Th28: A combined spectroscopic study with MUSE and X-Shooter | ||
The role of initial protostellar disk on the chemical evolution of the disk | ||
Radiation-hydrodynamical simulations of photoevaporating protoplanetary disks with various metallicities | ||
Is it really true that classical T Tauri stars evolve into weak-lined T Tauri stars? | ||
A study of the cold cores population of the star forming region in Perseus | ||
A Herschel survey of outbursting sources | ||
The dynamics of a young protostellar core | ||
First large-scale Herbig Haro jet driven by a proto-brown dwarf | ||
A survey of prestellar, high-mass cluster-forming clumps: Constraining models of high-mass star formation | ||
The formation of high-mass binary systems by core/disk fragmentation: Early results | ||
ALMA resolves a massive disk around an O-type YSO | ||
Simulations of stellar jets with magnetospheric accretion in T Tauris | ||
HST and Chandra observations of the RY Tau jet | ||
Infrared variability and the activity of masers - The case of G107.298+5.639 | ||
Near-IR & optical monitoring campaign of active young stars: Understanding the mechanism of jet launching | ||
Planet formation in AB Aurigae: Imaging of the inner gaseous spirals observed inside the dust cavity | ||
Accretion dynamics in pre-main sequence binaries | ||
Grand design spiral arms in a young forming circumstellar disk | ||
Herbig Ae/Be stars with TGAS parallaxes in the HR diagram | ||
Investigating the LVC with spectro-astrometry | ||
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Phase-space structure in the Monoceros region: Radial velocities and TGAS data | ||
The stellar content of the infalling molecular clump G286.21+0.17 | ||
Elemental abundances in star-forming regions | ||
The Gaia-ESO Survey: kinematical and dynamical study of four young open clusters | ||
Strӧmgren-Hβ photometry and optical polarization study of young open clusters | ||
Super star cluster forming cloud in the young and nearby starburst galaxy NGC5253 | ||
Towards solving the mistery of the "Seagull" nebula | ||
Kinematics in the early stages of star cluster formation | ||
The clustering properties of intermediate mass young stars | ||
Ages and distances to star forming regions from the synergy of X-rays and IR observations | ||
The impact of a star-formation efficiency profile on the evolution of open clusters | ||
Photometric determination of the system-IMF of the 25 Orionis stellar group | ||
Star formation toward IRAS 10427-6032, an H II region in the outskirts of the Carina Nebula | ||
Age spread and sequential star formation in the young cluster NGC 2264 | ||
Modeling stellar cluster formation in the presence of feedback | ||
The dynamics of star clusters and OB associations | ||
X-rays from young clusters reveal binarity of massive stars | ||
Tracing intermediate/low mass young stellar populations in the Magellanic Cloud | ||
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Accurate determination of radiation damped profiles in the reionization epoch | ||
Formation environment of Pop II stars affected by the feedbacks from Pop III stars | ||
Tracing molecular cloud formation with [CII] and [CI] | ||
Star formation thourgh cosmic space and time as traced by Milky Way progenitors | ||
Supernovae: Dust in the early universe and impact to star formation | ||
Supermassive star formation with detailed modelling of primordial-gas chemistry | ||
Stellar wind prevents the ISM gas from accreting onto the popIII stars | ||
A tale of Population III star formation: discussion of key physical parameters and roads to massive stars |