activity
20102023
most citedHerschel Measurements of Molecular Oxygen in Orion

170 citations · 1.6k across the 33 of their papers we have counts for

collaborators

33 papers

astro-ph.SR2023★ 20 cited

Brightness and mass accretion rate evolution during the 2022 burst of EX~Lupi

F. Cruz-Sáenz de Miera, Á. Kóspál, P. Ábrahám +18

EX Lupi is the prototype by which EXor-type outbursts were defined. It has experienced multiple accretion-related bursts and outbursts throughout the last decades, whose study have…

astro-ph.SR2023★ 14 cited

Gaia21bty: An EXor lightcurve exhibiting an FUor spectrum

Michał Siwak, Lynne A. Hillenbrand, Ágnes Kóspál +16

Gaia21bty, a pre-main sequence star that previously had shown aperiodic dips in its light curve, underwent a considerable mag brightening that occurred over a few mo…

astro-ph.SR2023★ 18 cited

The Gaia alerted fading of the FUor-type star Gaia21elv

Zsófia Nagy, Sunkyung Park, Péter Ábrahám +26

FU Orionis objects (FUors) are eruptive young stars, which exhibit outbursts that last from decades to a century. Due to the duration of their outbursts, and to the fact that only…

astro-ph.SR2022★ 18 cited

Photometric and spectroscopic study of the EXor-like eruptive young star Gaia19fct

Sunkyung Park, Ágnes Kóspál, Péter Ábrahám +19

Gaia19fct is one of the Gaia-alerted eruptive young stars that has undergone several brightening events. We conducted monitoring observations using multi-filter optical and near-in…

astro-ph.SR2022★ 5 cited

Photometric and spectroscopic study of the burst-like brightening of two Gaia-alerted young stellar objects

Zsófia Nagy, Péter Ábrahám, Ágnes Kóspál +18

Young stars show variability on different time-scales from hours to decades, with a range of amplitudes. We studied two young stars, which triggered the Gaia Science Alerts system…

astro-ph.SR2022★ 143 cited

Gaia Data Release 3. Summary of the variability processing and analysis

L. Eyer, M. Audard, B. Holl +55

Context. Gaia has been in operations since 2014. The third Gaia data release expands from the early data release (EDR3) in 2020 by providing 34 months of multi-epoch observations t…

astro-ph.SR2022

Episodic ejection from a low-mass young stellar object traced by HO masers

Zs. M. Szabó, O. Bayandina, Á. Kóspál +5

We present the project of a VLBI study of the 22 GHz HO maser in a prototypical low-mass protostellar system IRAS 16293-2422. The observation was conducted to characterise the…

astro-ph.SR2021★ 18 cited

Recurrent strong outbursts of an EXor-like young eruptive star Gaia20eae

Fernando Cruz-Sáenz de Miera, Ágnes Kóspál, Péter Ábrahám +21

We present follow-up photometric and spectroscopic observations, and subsequent analysis of Gaia20eae. This source triggered photometric alerts during 2020 after showing a 3…

astro-ph.IM2021★ 134 cited

Gaia Photometric Science Alerts

S. T. Hodgkin, D. L. Harrison, E. Breedt +108

Since July 2014, the Gaia mission has been engaged in a high-spatial-resolution, time-resolved, precise, accurate astrometric, and photometric survey of the entire sky. Aims: We pr…

astro-ph.SR2021★ 8 cited

Dipper-like variability of the Gaia alerted young star V555 Ori

Zsófia Nagy, Elza Szegedi-Elek, Péter Ábrahám +26

V555 Ori is a T Tauri star, whose 1.5 mag brightening was published as a Gaia science alert in 2017. We carried out optical and near-infrared photometric, and optical spectroscopic…

astro-ph.GA2021★ 32 cited

An HST Survey of Protostellar Outflow Cavities: Does Feedback Clear Envelopes?

Nolan M. Habel, S. Thomas Megeath, Joseph Jon Booker +10

We study protostellar envelope and outflow evolution using Hubble Space Telescope NICMOS or WFC3 images of 304 protostars in the Orion Molecular clouds. These near-IR images resolv…

astro-ph.SR2020★ 10 cited

Constraining the Chemical Signatures and the Outburst Mechanism of the Class 0 Protostar HOPS 383

Rajeeb Sharma, John J. Tobin, Patrick D. Sheehan +5

We present observations toward HOPS 383, the first known outbursting Class 0 protostar located within the Orion molecular cloud using ALMA, VLA, and SMA. The SMA observations revea…

astro-ph.GA2020★ 27 cited

Distribution of methanol and cyclopropenylidene around starless cores

S. Spezzano, P. Caselli, J. E. Pineda +3

Context. The spatial distribution of molecules around starless cores is a powerful tool for studying the physics and chemistry governing the earliest stages of star formation. Aims…

astro-ph.GA2020★ 11 cited

An APEX survey of outflow and infall toward the youngest protostars in Orion

Z. Nagy, A. Menechella, S. T. Megeath +7

We aim to characterize the outflow properties of a sample of early Class 0 phase low-mass protostars in Orion first identified by the Herschel Space Observatory. We also look for s…

astro-ph.GA2019★ 34 cited

The chemical structure of the very young starless core L1521E

Z. Nagy, S. Spezzano, P. Caselli +5

L1521E is a dense starless core in Taurus that was found to have relatively low molecular depletion by earlier studies, thus suggesting a recent formation. We aim to characterize t…

astro-ph.GA2018★ 104 cited

Structure of photodissociation fronts in star-forming regions revealed by observations of high-J CO emission lines with Herschel

C. Joblin, E. Bron, C. Pinto +17

In bright photodissociation regions (PDRs) associated to massive star formation, the presence of dense "clumps" that are immersed in a less dense interclump medium is often propose…

astro-ph.GA2016★ 37 cited

Herschel / HIFI spectral line survey of the Orion Bar - Temperature and density differentiation near the PDR surface

Z. Nagy, Y. Choi, V. Ossenkopf-Okada +7

Photon Dominated Regions (PDRs) are interfaces between the mainly ionized and mainly molecular material around young massive stars. Analysis of the physical and chemical structure…

astro-ph.GA2016★ 24 cited

Characterizing the Youngest Herschel-detected Protostars II. Molecular Outflows from the Millimeter and the Far-infrared

John J. Tobin, Amelia M. Stutz, P. Manoj +7

We present CARMA CO (J=1-0) observations and Herschel PACS spectroscopy, characterizing the outflow properties toward extremely young and deeply embedded protostars in the Orion mo…

astro-ph.GA2016★ 29 cited

Herschel/HIFI Spectral Mapping of C, CH, and CH in Orion BN/KL: The Prevailing Role of Ultraviolet Irradiation in CH Formation

Patrick W. Morris, Harshal Gupta, Zsofia Nagy +8

The CH ion is a key species in the initial steps of interstellar carbon chemistry. Its formation in diverse environments where it is observed is not well understood, however, b…

astro-ph.SR2016★ 36 cited

Observations and modelling of CO and [CI] in disks. First detections of [CI] and constraints on the carbon abundance

M. Kama, S. Bruderer, M. Carney +23

The gas-solid budget of carbon in protoplanetary disks is related to the composition of the cores and atmospheres of the planets forming in them. The key gas-phase carbon carriers…

astro-ph.SR2015★ 19 cited

Outflow forces in intermediate mass star formation

T. A. van Kempen, M. R. Hogerheijde, E. F. van Dishoeck +22

Intermediate mass protostarsprovide a bridge between theories of low- and high-mass star formation. Emerging molecular outflows can be used to determine the influence of fragmentat…

astro-ph.GA2015★ 18 cited

Physical and chemical differentiation of the luminous star-forming region W49A - Results from the JCMT Spectral Legacy Survey

Z. Nagy, F. F. S. van der Tak, G. A. Fuller +1

The massive and luminous star-forming region W49A is a well known Galactic candidate to probe the physical conditions and chemistry similar to those expected in external starburst…

astro-ph.SR2015★ 107 cited

APEX-CHAMP+ high-J CO observations of low-mass young stellar objects: IV. Mechanical and radiative feedback

Umut A. Yıldız, Lars E. Kristensen, Ewine F. van Dishoeck +14

During the embedded stage of star formation, bipolar molecular outflows and UV radiation from the protostar are important feedback processes. Our aim is to quantify the feedback, m…

astro-ph.GA2014★ 47 cited

CH observations toward the Orion Bar

Z. Nagy, V. Ossenkopf, F. F. S. Van der Tak +3

CH is one of the first radicals to be detected in the interstellar medium. Its higher rotational transitions have recently become available with the Herschel Space Observatory.…