activity
20072017
most citedA Major Asymmetric Dust Trap in a Transition Disk

611 citations · 2k across the 20 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2016★ 16 cited

The Herschel-HIFI view of mid-IR quiet massive protostellar objects

F. Herpin, L. Chavarria, T. Jacq +9

We present Herschel/HIFI observations (WISH KP) of 14 water lines in a small sample of galactic massive protostellar objects: NGC6334I(N), DR21(OH), IRAS16272-4837, and IRAS05358+3…

astro-ph.SR2013★ 50 cited

ALMA continuum observations of a 30 Myr old gaseous debris disk around HD 21997

A. Moór, A. Juhász, Á. Kóspál +10

Circumstellar disks around stars older than 10 Myr are expected to be gas-poor. There are, however, two examples of old (30-40 Myr) debris-like disks containing a detectable amount…

astro-ph.SR2013★ 140 cited

ALMA observations of the molecular gas in the debris disk of the 30 Myr old star HD 21997

Á. Kóspál, A. Moór, A. Juhász +9

The 30 Myr old A3-type star HD 21997 is one of the two known debris dust disks having a measurable amount of cold molecular gas. With the goal of understanding the physical state,…

astro-ph.SR2013★ 63 cited

Gas-phase CO depletion and N2H+ abundances in starless cores

N. Lippok, R. Launhardt, D. Semenov +10

Seven isolated, nearby low-mass starless molecular cloud cores have been observed as part of the Herschel key program Earliest Phases of Star formation (EPoS). By applying a ray-tr…

astro-ph.SR2013★ 169 cited

The earliest phases of star formation - A Herschel key project. The thermal structure of low-mass molecular cloud cores

R. Launhardt, A. M. Stutz, A. Schmiedeke +19

The temperature and density structure of molecular cloud cores are the most important physical quantities that determine the course of the protostellar collapse and the properties…

astro-ph.SR2012★ 46 cited

ALMA CO J=6-5 observations of IRAS16293-2422: Shocks and entrainment

L. E. Kristensen, P. D. Klaassen, J. C. Mottram +2

Observations of higher-excited transitions of abundant molecules such as CO are important for determining where energy in the form of shocks is fed back into the parental envelope…

astro-ph.SR2012★ 288 cited

Detection of the simplest sugar, glycolaldehyde, in a solar-type protostar with ALMA

Jes K. Jorgensen, Cecile Favre, Suzanne E. Bisschop +3

Glycolaldehyde (HCOCH2OH) is the simplest sugar and an important intermediate in the path toward forming more complex biologically relevant molecules. In this paper we present the…

astro-ph.SR2012★ 47 cited

SMA and Spitzer Observations of Bok Glouble CB17: A Candidate First Hydrostatic Core?

Xuepeng Chen, Hector G. Arce, Michael M. Dunham +5

We present high angular resolution SMA and Spitzer observations toward the Bok globule CB17. SMA 1.3mm dust continuum images reveal within CB17 two sources with an angular separati…

astro-ph.SR2010★ 89 cited

L1448 IRS2E: A candidate first hydrostatic core

Xuepeng Chen, Hector G. Arce, Qizhou Zhang +4

Intermediate between the prestellar and Class 0 protostellar phases, the first core is a quasi-equilibrium hydrostatic object with a short lifetime and an extremely low luminosity.…