activity
20082024
most citedConsistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs

379 citations · 1.1k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.IM2024★ 15 cited

The new Herschel/PACS Point Source Catalogue

Gábor Marton, Ilknur Gezer, Máté Madarász +6

Herschel operated as an observatory, therefore it did not cover the whole sky, but still observed ~8% of it. The first version of an overall Herschel/PACS Point Source Catalogue wa…

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.SR2020★ 12 cited

Feedback of molecular outflows from protostars in NGC 1333, revealed by Herschel and Spitzer spectro-imaging observations

Odysseas Dionatos, Lars. E. Kristensen, Mario Tafalla +2

Large scale spectral maps of star forming regions enable the comparative study of the gas excitation around an ensemble of sources at a common frame of reference, providing direct…

astro-ph.SR2019★ 2 cited

Infrared and sub-mm observations of outbursting young stars with Herschel and Spitzer

Andreas Postel, Marc Audard, Eduard Vorobyov +3

Episodic accretion plays an important role in the evolution of young stars. Although it has been under investigation for a long time, the origin of such episodic accretion events i…

astro-ph.SR2019★ 32 cited

Consistent dust and gas models for protoplanetary disks IV. A panchromatic view of protoplanetary disks

O. Dionatos, P. Woitke, M. Guedel +17

Consistent modeling of protoplanetary disks requires the simultaneous solution of both continuum and line radiative transfer, heating/cooling balance between dust and gas and, of c…

astro-ph.EP2018★ 93 cited

Consistent dust and gas models for protoplanetary disks III. Models for selected objects from the FP7 DIANA project

P. Woitke, I. Kamp, S. Antonellini +17

The European FP7 project DIANA has performed a coherent analysis of a large set of observations from protoplanetary disks by means of thermo-chemical disk models. The collected dat…

astro-ph.SR2018

Discovery of a primordial water reservoir in the envelope of HH211

Odysseas Dionatos

We report on the detection of a rich water reservoir in the protostellar envelope of the Class 0 source HH211. In striking contrast to all other molecules detected with Herschel/PA…

astro-ph.SR2018★ 31 cited

ALMA detects a radial disk wind in DG Tau

M. Guedel, C. Eibensteiner, O. Dionatos +7

Aims: We aim to use the high spatial resolution of the Atacama Large Millimeter/submillimeter Array (ALMA) to map the flow pattern of molecular gas near DG Tau and its disk, a youn…

astro-ph.SR2018★ 12 cited

Herschel spectral-line mapping of the HH211 protostellar system

Odysseas Dionatos, Tom Ray, Manuel Guedel

(Abridged) Mid- and far-infrared observations of the environment around embedded protostars reveal a plethora of high excitation molecular and atomic emission lines. In this work w…

astro-ph.GA2018★ 31 cited

CO in Protostars (COPS): -SPIRE Spectroscopy of Embedded Protostars

Yao-Lun Yang, Joel D. Green, Neal J. Evans +13

We present full spectral scans from 200-670m of 26 Class 0+I protostellar sources, obtained with -SPIRE, as part of the "COPS-SPIRE" Open Time program, complementary t…

astro-ph.SR2017★ 53 cited

The chemistry of episodic accretion in embedded objects. 2D radiation thermo-chemical models of the post-burst phase

Ch. Rab, V. Elbakyan, E. Vorobyov +7

Episodic accretion is an important process in the evolution of young stars and their environment. The observed strong luminosity bursts of young stellar objects likely have a long…

astro-ph.EP2016★ 8 cited

The gas disk: Evolution and chemistry

Ch. Rab, C. Baldovin-Saavedra, O. Dionatos +2

Protoplanetary disks are the birthplaces of planetary systems. The evolution of the star-disk system and the disk chemical composition determines the initial conditions for planet…

astro-ph.SR2016★ 22 cited

The feedback of atomic jets from embedded protostars in NGC 1333

Odysseas Dionatos, Manuel Güdel

Star-formation feedback onto the parent cloud is conventionally examined through the study of molecular outflows. Little is however known on the effect that atomic ejecta, tracing…

astro-ph.EP2015★ 379 cited

Consistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs

P. Woitke, M. Min, C. Pinte +19

We propose a set of standard assumptions for the modelling of Class II and III protoplanetary disks, which includes detailed continuum radiative transfer, thermo-chemical modelling…

astro-ph.GA2014★ 23 cited

Atomic jet from SMM1 (FIRS1) in Serpens uncovers non-coeval binary companion

O. Dionatos, J. K. Jørgensen, P. S. Teixeira +2

We report on the detection of an atomic jet associated with the protostellar source SMM1 (FIRS1) in Serpens. The jet is revealed in [FeII] and [NeII] line maps observed with Spitze…

astro-ph.SR2013★ 30 cited

Warm gas towards young stellar objects in Corona Australis - Herschel/PACS observations from the DIGIT key programme

Johan E. Lindberg, Jes K. Jørgensen, Joel D. Green +5

The effects of external irradiation on the chemistry and physics in the protostellar envelope around low-mass young stellar objects are poorly understood. The Corona Australis star…

astro-ph.GA2013★ 21 cited

L1448-MM observations by the Herschel Key program, "Dust, Ice, and Gas In Time" (DIGIT)

Jinhee Lee, Jeong-Eun Lee, Seokho Lee +7

We present Herschel/PACS observations of L1448-MM, a Class 0 protostar with a prominent outflow. Numerous emission lines are detected at 55 < lambda < 210 micrometer including CO,…

astro-ph.GA2013★ 31 cited

DIGIT: Herschel and Spitzer spectro-imaging of SMM3 and SMM4 in Serpens

O. Dionatos, J. K. Jørgensen, J. D. Green +5

We report on spectro-imaging observations employing Spitzer IRS and Herschel PACS, aiming to constrain the physical conditions around SMM3 and SMM4 in Serpens. The combined power o…

astro-ph.GA2013★ 126 cited

Embedded Protostars in the Dust, Ice, and Gas In Time (DIGIT) Key Program: Continuum SEDs, and an Inventory of Characteristic Far-Infrared Lines from PACS Spectroscopy

Joel D. Green, Neal J. Evans, Jes K. Jørgensen +17

We present 50-210 um spectral scans of 30 Class 0/I protostellar sources, obtained with Herschel-PACS, and 0.5-1000 um SEDs, as part of the Dust, Ice, and Gas in Time (DIGIT) Key P…

astro-ph.GA2011★ 30 cited

Herschel observations of the Herbig-Haro objects HH52-54

P. Bjerkeli, R. Liseau, B. Nisini +11

We are aiming at the observational estimation of the relative contribution to the cooling by CO and H2O, as this provides decisive information for the understanding of the oxygen c…

astro-ph.GA2010★ 25 cited

Wide field CO J = 3->2 mapping of the Serpens Cloud Core

O. Dionatos, B. Nisini, C. Codella +1

Context. Outflows provide indirect means to get an insight on diverse star formation associated phenomena. On scales of individual protostellar cores, outflows combined with intrin…

astro-ph.GA2010★ 41 cited

Spitzer spectral line mapping of the HH211 outflow

O. Dionatos, B. Nisini, S. Cabrit +2

Aims: We employ archival Spitzer slit-scan observations of the HH211 outflow in order to investigate its warm gas content, assess the jet mass flux in the form of H2 and probe for…

astro-ph2008★ 47 cited

Atomic jets from class 0 sources detected by Spitzer: the case of L1448-C

O. Dionatos, B. Nisini, R. Garcia Lopez +5

We present Spitzer-IRS spectra obtained along the molecular jet from the Class 0 source L1448-C (or L1448-mm). Atomic lines from the fundamental transitions of [FeII], [SiII] and […