The Atacama Pathfinder EXperiment (APEX)–a new submillimeter facility for southern skies–

R Güsten, LÅ Nyman, P Schilke, K Menten… - Astronomy & …, 2006 - aanda.org
APEX, the Atacama Pathfinder EXperiment, has been successfully commissioned and is
operational. This novel submillimeter telescope is located at 5107 m altitude on Llano de …

A Swedish heterodyne facility instrument for the APEX telescope

V Vassilev, D Meledin, I Lapkin, V Belitsky… - Astronomy & …, 2008 - aanda.org
Aims. In March 2008, the APEX facility instrument was installed on the telescope at the site
of Lliano Chajnantor in northern Chile. The main objective of the paper is to introduce the …

Extended rotating disks around post-AGB stars

V Bujarrabal, J Alcolea, H Van Winckel… - Astronomy & …, 2013 - aanda.org
Context. There is a group of binary post-AGB stars that show conspicuous near-infrared
(NIR) excess, which is usually assumed to arise from hot dust in very compact possibly …

SEPIA345: A 345 GHz dual polarization heterodyne receiver channel for SEPIA at the APEX telescope

D Meledin, I Lapkin, M Fredrixon, E Sundin… - Astronomy & …, 2022 - aanda.org
Context. We describe the new SEPIA345 heterodyne receiver channel installed at the
Atacama Pathfinder EXperiment (APEX) telescope, including details of its configuration …

Deuterium chemistry in the Orion Bar PDR-“Warm” chemistry starring CH2D+

B Parise, S Leurini, P Schilke, E Roueff… - Astronomy & …, 2009 - aanda.org
Context. High levels of deuterium fractionation in gas-phase molecules are usually
associated with cold regions, such as prestellar cores. Significant fractionation ratios are …

Initial phases of massive star formation in high infrared extinction clouds-I. Physical parameters

KLJ Rygl, F Wyrowski, F Schuller… - Astronomy & …, 2010 - aanda.org
Aims. The earliest phases of massive star formation are found in cold and dense infrared
dark clouds (IRDCs). Since the detection method of IRDCs is very sensitive to the local …

Abundances and Isotope Ratios in the Magellanic Clouds: The Star-Forming Environment of N 113

M Wang, YN Chin, C Henkel, JB Whiteoak… - The Astrophysical …, 2008 - iopscience.iop.org
With the goal of deriving the physical and chemical conditions of star-forming regions in the
Large Magellanic Cloud (LMC), a spectral line survey of the prominent star-forming region N …

Dense and warm molecular gas in the envelopes and outflows of southern low-mass protostars

TA van Kempen, EF van Dishoeck… - Astronomy & …, 2009 - aanda.org
Context. Observations of dense molecular gas lie at the basis of our understanding of the
density and temperature structure of protostellar envelopes and molecular outflows. The …

THz low resolution spectroscopy for astronomy

GJ Stacey - IEEE Transactions on Terahertz Science and …, 2011 - ieeexplore.ieee.org
The THz spectral regime provides a wide range of spectral lines that are invaluable probes
of star formation and AGN activity in galaxies both in the local Universe and at the earliest …

Extended emission of D2H+ in a prestellar core

B Parise, A Belloche, F Du, R Güsten… - Astronomy & …, 2011 - aanda.org
Context. In the past years, the H 2 D+ and D 2 H+ molecules have gained attention as
probes of cold and depleted dense molecular cloud cores. These ions are the basis of …