activity
20182021
most citedThe CO-dark molecular gas mass in 30 Doradus

44 citations · 114 across the 6 of their papers we have counts for

collaborators

10 papers

astro-ph.SR202111 cited

Evolution of the atomic component in protostellar outflows

T. Sperling, J. Eislöffel, B. Nisini +3

We present SOFIA/FIFI-LS observations of three Class 0 and one Class I outflows (Cep E, HH 1, HH 212, and L1551 IRS5) in the far-infrared [O I]63mum and [O I]145mum transitions. Sp…

astro-ph.SR20211 cited

Infrared observations of the flaring maser source G358.93-0.03 -- SOFIA confirms an accretion burst from a massive young stellar object

B. Stecklum, V. Wolf, H. Linz +24

Class II methanol masers are signs of massive young stellar objects (MYSOs). Recent findings show that MYSO accretion bursts cause flares of these masers. Thus, maser monitoring ca…

astro-ph.GA20209 cited

A SOFIA Survey of [CII] in the galaxy M51 II. [CII] and CO kinematics across spiral arms

Jorge L. Pineda, Juergen Stutzki, Christof Buchbender +10

We present the first complete, velocity-resolved [CII] 158um image of the M51 grand-design spiral galaxy, observed with the upGREAT instrument on SOFIA. [CII] is an important trace…

astro-ph.GA202044 cited

The CO-dark molecular gas mass in 30 Doradus

Mélanie Chevance, Suzanne C. Madden, Christian Fischer +16

Determining the efficiency with which gas is converted into stars in galaxies requires an accurate determination of the total reservoir of molecular gas mass. However, despite bein…

astro-ph.GA201914 cited

The Close AGN Reference Survey (CARS). Discovery of a global [CII] 158 m line excess in AGN HE1353-1917

I. Smirnova-Pinchukova, B. Husemann, G. Busch +15

The [CII]158m line is one of the strongest far-infrared (FIR) lines and an important coolant in the interstellar medium of galaxies that is accessible out to high redshifts. The…

astro-ph.SR201935 cited

Time-variable electromagnetic star-planet interaction: The TRAPPIST-1 system as an exemplary case

Christian Fischer, Joachim Saur

Exoplanets sufficiently close to their host star can in principle couple electrodynamically to the star. This process is known as electrodynamic star-planet interaction (SPI). The…