681 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR190 papers
- Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresFR83 papers
- Max Planck Institute for AstronomyDE82 papers
- Sorbonne UniversitéFR77 papers
- Université Paris Sciences et LettresFR75 papers
- National Radio Astronomy ObservatoryUS74 papers
- Laboratoire d'Astrophysique de BordeauxFR65 papers
- Université de BordeauxFR63 papers
- Institut de Recherche en Astrophysique et PlanétologieFR59 papers
- Center for Astrophysics Harvard & SmithsonianUS58 papers
- Max Planck Institute for Radio AstronomyDE53 papers
- Université Grenoble AlpesFR53 papers
56 papers · 1 filter
Rotating molecular outflows: the young T Tauri star in CB26
R. Launhardt, Ya. Pavlyuchenkov, F. Gueth +7
The disk-outflow connection is thought to play a key role in extracting excess angular momentum from a forming proto-star. Though jet rotation has been observed in a few objects, n…
HCO mapping of the Horsehead : Tracing the illuminated dense molecular cloud surfaces
Maryvonne Gerin, Javier R. Goicoechea, Jérôme Pety +1
Far-UV photons strongly affect the physical and chemical state of molecular gas in the vicinity of young massive stars. We have obtained maps of the HCO and H13CO+ ground state lin…
The CO line SED and atomic carbon in IRAS F10214+4724
Y. Ao, A. Weiss, D. Downes +3
Using the IRAM 30m telescope and the Plateau de Bure interferometer we have detected the \ctwo and the CO 32, 43, 65, 76 transitions as well as the dust continuum at 3…
Ram-pressure stripped molecular gas in the Virgo spiral galaxy NGC 4522
B. Vollmer, J. Braine, C. Pappalardo +1
IRAM 30m 12CO(1-0) and 12CO(2-1) HERA observations are presented for the ram-pressure stripped Virgo spiral galaxy NGC 4522. The CO emission is detected in the galactic disk and th…
Chemistry in Disks. II. -- Poor molecular content of the AB Aur disk
Katharina Schreyer, Stéphane Guilloteau, Dmitry Semenov +9
We study the molecular content and chemistry of a circumstellar disk surrounding the Herbig Ae star AB Aur at (sub-)millimeter wavelengths. Our aim is to reconstruct the chemical h…
HI and CO in the circumstellar environment of the oxygen-rich AGB star RX Lep
Y. Libert, T. Le Bertre, E. Gérard +1
Circumstellar shells around AGB stars are built over long periods of time that may reach several million years. They may therefore be extended over large sizes (~1 pc, possibly mor…
Gas flow models in the Milky Way embedded bars
Nemesio Rodriguez-Fernandez, Francoise Combes
The gas distribution and dynamics in the inner Galaxy present many unknowns as the origin of the asymmetry of the longitude-velocity (lv) diagram of the Central Molecular Zone (CMZ…
Disks around CQ Tau and MWC 758: dense PDR or gas dispersal?
Edwige Chapillon, Stéphane Guilloteau, Anne Dutrey +1
The overall properties of disks surrounding intermediate PMS stars (HAe) are not yet well constrained by current observations. The disk inclination, which significantly affect SED…
Cold gas in the Perseus cluster core: Excitation of molecular gas in filaments
P. Salomé, F. Combes, Y. Revaz +4
We have recently detected CO lines in the well-known filaments around NGC 1275, the galaxy at the centre of the Perseus cluster of galaxies. These previous observations, with the H…
Long-term observations of Uranus and Neptune at 90 GHz with the IRAM 30m telescope - (1985 -- 2005)
C. Kramer, R. Moreno, A. Greve
The planets Uranus and Neptune with small apparent diameters are primary calibration standards. We investigate their variability at ~90 GHz using archived data taken at the IRAM 30…
CN in prestellar cores
Pierre Hily-Blant, Malcolm Walmsley, G. Pineau Des Forêts +1
Determining the structure of and the velocity field in prestellar cores is essential to understanding protostellar evolution.} {We have observed the dense prestellar cores L 1544 a…
The Horsehead mane: Towards an observational benchmark for chemical models
Jérôme Pety, Javier R. Goicoechea, Maryvonne Gerin +5
After a discussion about the need for observational benchmark for chemical models, we explain 1) why the Horsehead western edge is well suited to serve as reference for models and…
Evidence for alignment of the rotation and velocity vectors in pulsars. II. Further data and emission heights
Simon Johnston, M. Kramer, A. Karastergiou +3
We have conducted observations of 22 pulsars at frequencies of 0.7, 1.4 and 3.1 GHz and present their polarization profiles. The observations were carried out for two main purposes…
The earliest phases of high-mass star formation: a 3 square degree millimeter continuum mapping of Cygnus X
Frédérique Motte, S. Bontemps, P. Schilke +3
We have made an extensive 1.2mm continuum mosaicing study of the Cygnus X molecular cloud complex using the MAMBO cameras at the IRAM 30 m telescope. We then compared our mm maps w…
Gravitational stability in the disk of M51
M. Hitschfeld, C. Kramer, K. F. Schuster +2
Star formation laws, like i.e. the Schmidt law relating star formation rate and total gas density, have been studied in several spiral galaxies but the underlying physics are not y…
Molecular gas in QSO host galaxies at z>5
R. Maiolino, R. Neri, A. Beelen +10
We present observations with the IRAM Plateau de Bure Interferometer of three QSOs at z>5 aimed at detecting molecular gas in their host galaxies as traced by CO transitions. CO (5…
Molecular line radiative transfer in protoplanetary disks: Monte Carlo simulations versus approximate methods
Ya. Pavlyuchenkov, D. Semenov, Th. Henning +4
We analyze the line radiative transfer in protoplanetary disks using several approximate methods and a well-tested Accelerated Monte Carlo code. A low-mass flaring disk model with…
An empirical model for the beams of radio pulsars
A. Karastergiou, S. Johnston
Motivated by recent results on the location of the radio emission in pulsar magnetospheres, we have developed a model which can account for the large diversity found in the average…
Particularly Efficient Star Formation in M33
E. Gardan, J. Braine, K. F. Schuster +2
The Star Formation (SF) rate in galaxies is an important parameter at all redshifts and evolutionary stages of galaxies. In order to understand the increased SF rates in intermedia…
Discovery of Interstellar Propylene (CH_2CHCH_3): Missing Links in Interstellar Gas-Phase Chemistry
N. Marcelino, J. Cernicharo, M. Agundez +5
We report the discovery of propylene (also called propene, CH_2CHCH_3) with the IRAM 30-m radio telescope toward the dark cloud TMC-1. Propylene is the most saturated hydrocarbon e…
Highly-excited CO emission in APM08279+5255 at z=3.9
A. Weiss, D. Downes, R. Neri +5
We report the detection of the CO 4-3, 6-5, 9-8, 10-9, and 11-10 lines in the Broad Absorption Line quasar APM08279+5255 at z=3.9 using the IRAM 30m telescope. We also present IRAM…
Small-scale dissipative structures of diffuse ISM turbulence: I- CO diagnostics
Pierre Hily-Blant, Jerome Pety, Edith Falgarone
Observations of translucent molecular gas in CO and CO emission lines, at high spectral and spatial resolutions, evidence different kinds of structures at small scale…
A highly-collimated SiO jet in the HH212 protostellar outflow
C. Codella, S. Cabrit, F. Gueth +4
We mapped the HH212 Class 0 outflow in SiO(2--1, 5--4) and continuum using the PdBI in its extended configurations. The unprecedented angular resolution (down to 0.34") allows accu…
Detection of HNC and tentative detection of CN at z=3.9
M. Guelin, P. Salome, R. Neri +8
Molecular line emission from high-redshift galaxies holds great promise for the study of galaxy formation and evolution. The weak signals can only be detected with the largest mm-w…