output
19942026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2013 · astro-ph.SRShow all

49 papers · 2 filters

astro-ph.SR2013★ 146 cited

Gas structure inside dust cavities of transition disks: Oph IRS 48 observed by ALMA

Simon Bruderer, Nienke van der Marel, Ewine F. van Dishoeck +1

(Abridged) Transition disks are recognized by the absence of emission of small dust grains inside a radius of up to several 10s of AUs. Due to the lack of angular resolution and se…

astro-ph.SR2013★ 122 cited

A recent accretion burst in the low-mass protostar IRAS 15398-3359: ALMA imaging of its related chemistry

Jes K. Jorgensen, Ruud Visser, Nami Sakai +8

Low-mass protostars have been suggested to show highly variable accretion rates through-out their evolution. Such changes in accretion, and related heating of their ambient envelop…

astro-ph.SR2013★ 56 cited

Far-infrared molecular lines from Low- to High-Mass Star Forming Regions observed with Herschel

A. Karska, F. Herpin, S. Bruderer +13

(Abridged) We study the response of the gas to energetic processes associated with high-mass star formation and compare it with studies on low- and intermediate-mass young stellar…

astro-ph.SR2013★ 16 cited

Imaging the circumstellar environment of the young T Tauri star SU Aurigae

S. V. Jeffers, M. Min, H. Canovas +2

The circumstellar environments of classical T Tauri stars are challenging to directly image because of their high star-to-disk contrast ratio. One method to overcome this is by usi…

astro-ph.SR2013★ 6 cited

Morphologies of protostellar outflows: An ALMA view

Thomas Peters, Pamela D. Klaassen, Daniel Seifried +2

The formation of stars is usually accompanied by the launching of protostellar outflows. Observations with the Atacama Large Millimetre/sub-millimetre Array (ALMA) will soon revolu…

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…