144 citations · 2.6k across the 65 of their papers we have counts for
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Characterising the multiple protostellar system VLA 1623-2417 with JWST, ALMA and VLA: outflow origins, dust growth and an unsettled disk
Isaac C. Radley, Gemma Busquet, John D. Ilee +16
Utilising JWST, ALMA and the VLA we present high angular resolution (0.06''- 0.42''), multi-wavelength (4 micron - 3cm) observations of the VLA 1623-2417 protostellar system to cha…
Evidence for Jet/Outflow Shocks Heating the Environment Around the Class I Protostellar Source Elias 29: FAUST XXI
Yoko Oya, Eri Saiga, Anna Miotello +1
We have observed the late Class I protostellar source Elias~29 at a spatial-resolution of 70~au with the Atacama~Large~Millimeter/submillimeter~Array (ALMA) as part of the FAUST La…
FAUST VIII. The protostellar disk of VLA 1623-2417 W and its streamers imaged by ALMA
S. Mercimek, L. Podio, C. Codella +25
More than 50% of solar-mass stars form in multiple systems. It is therefore crucial to investigate how multiplicity affects the star and planet formation processes at the protostel…
Chemical and Physical Characterization of the Isolated Protostellar Source CB68: FAUST. IV
Muneaki Imai, Yoko Oya, Brian Svoboda +1
Chemical diversity of low-mass protostellar sources has so far been recognized, and environmental effects are invoked as its origin. In this context, observations of isolated proto…
Modeling the accretion disk around the high-mass protostar GGD 27-MM1
N. Añez-Lopez, M. Osorio, G. Busquet +9
Recent high-angular resolution (40 mas) ALMA observations at 1.14 mm resolve a compact (R~200 au) flattened dust structure perpendicular to the HH 80-81 jet emanating from the GGD…
Unveiling a cluster of protostellar disks around the massive protostar GGD27 MM1
G. Busquet, J. M. Girart, R. Estalella +9
We used ALMA to observe the star-forming region GGD27 at 1.14 mm with an unprecedented angular resolution, 40 mas (56 au) and sensitivity (0.002 Msun). We detected a cluster of 25…
Extreme fragmentation and complex kinematics at the center of the L1287 cloud
Carmen Juárez, Hauyu-Baobab Liu, Josep M. Girart +5
The filamentary infrared dark cloud L1287 is actively forming a dense cluster of low-mass YSOs at its inner 0.1 pc region. To help understand the origin of this low-mass YSO…
Distribution of Serpens South protostars revealed with ALMA
Adele L. Plunkett, Manuel Fernández-López, Héctor G. Arce +3
Aims: We investigated the masses and spatial distributions of pre-stellar and protostellar candidates in the young, low-mass star forming region Serpens South, where active star fo…
The circumestellar disk of the B0 protostar powering the HH 80-81 radio jet
J. M. Girart, R. Estalella, M. Fernández-López +6
We present subarcsecond angular resolution observations carried out with the Submillimeter Array (SMA) at 880 m centered at the B0-type protostar GGD27~MM1, the driving source o…
Ongoing star formation in the proto-cluster IRAS 22134+5834
Yuan Wang, Marc Audard, Francesco Fontani +9
IRAS 22134+5834 was observed in the centimeter with (E)VLA, 3~mm with CARMA, 2~mm with PdBI, and 1.3~mm with SMA, to study the continuum emission as well as the molecular lines, th…
Deuteration and evolution in the massive star formation process: the role of surface chemistry
F. Fontani, G. Busquet, Aina Palau +5
An ever growing number of observational and theoretical evidence suggests that the deuterated fraction (column density ratio between a species containing D and its hydrogenated cou…
The identification of filaments on far infrared and submillimiter images. Morphology, physical conditions and relation with star formation of filamentary structure
E. Schisano, K. L. Rygl, S. Molinari +12
Observations of molecular clouds reveal a complex structure, with gas and dust often arranged in filamentary rather than spherical geometries. The associations of pre- and proto- s…
The CHESS survey of the L1157-B1 shock region: CO spectral signatures of jet-driven bowshocks
B. Lefloch, S. Cabrit, G. Busquet +7
The unprecedented sensitivity of Herschel coupled with the high resolution of the HIFI spectrometer permits studies of the intensity-velocity relationship I(v) in molecular outflow…