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Related papers: First CH$_{3}$D detection in Class 0/I proto-brown…

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Studies of brown dwarf (BD) outflows provide information pertinent to questions on BD formation, as well as allowing outflow mechanisms to be investigated at the lowest masses. Here new observations of the bipolar outflow from the 24…

Solar and Stellar Astrophysics · Physics 2015-06-11 Emma Whelan , Tom Ray , Fernando Comeron , Francesca Bacciotti , Patrick Kavanagh

We observe 84 candidate young high-mass sources in the rare isotopologues C17O and C18O to investigate whether there is evidence for depletion (freeze-out) towards these objects. Observations of the J=2-1 transitions of C18O and C17O are…

Astrophysics · Physics 2009-11-13 H. S. Thomas , G. A. Fuller

Ethylene oxide (c-C$_{2}$H$_{4}$O) and its isomer, acetaldehyde (CH$_{3}$CHO), are important complex organic molecules owing to their potential role in the formation of amino acids (R-CH(NH$_{2}$)-COOH) in ISM. The detection of…

Astrophysics of Galaxies · Physics 2025-09-04 Arijit Manna , Sabyasachi Pal

The gas-solid budget of carbon in protoplanetary disks is related to the composition of the cores and atmospheres of the planets forming in them. The key gas-phase carbon carriers CO, C$^{0}$ and C$^{+}$ can now be observed in disks. The…

We report on the tentative detection of $trans$ Ethyl Methyl Ether (tEME), $t-CH_3CH_2OCH_3$, through the identification of a large number of rotational lines from each one of the spin states of the molecule towards Orion KL. We also search…

Absorption and emission lines originating from the nu3 C-H stretching manifold of gas phase CH4 were discovered in the high resolution (R=25,000) infrared L band spectrum along the line of sight toward NGC 7538 : IRS9. These observations…

Astrophysics · Physics 2016-08-30 A. C. A. Boogert , G. A. Blake , K. Oberg

We report new infrared spectroscopic observations of cool DQ white dwarfs by using Coolspec on the 2.7m Harlan-Smith Telescope. DQs have helium-rich atmospheres with traces of molecular carbon thought to be the result of convective…

Astrophysics · Physics 2007-05-23 M. Kilic , D. E. Winget , T. von Hippel , D. F. Lester , D. Saumon

High quality archival spectra of interstellar absorption from C I toward 9 stars, taken with the Goddard High Resolution Spectrograph on the Hubble Space Telescope, were analyzed. Our sample was supplemented by two sight lines, 23 Ori and…

Astrophysics · Physics 2009-11-07 J. Zsargo , S. R. Federman

We report high angular resolution (~0.6''x0.5'' at 1.3mm) observations of the Class 0 intermediate-mass (IM) protostar NGC 7129--FIRS 2 using the PdBI. Our observations show the existence of a hot core at the position of the Class 0 object.…

Astrophysics · Physics 2009-11-11 A. Fuente , R. Neri , P. Caselli

In an attempt to study whether the formation of brown dwarfs (BDs) takes place as a scaled-down version of low-mass stars, we conducted IRAM30m/MAMBO-II observations at 1.2 mm in a sample of 12 proto-BD candidates selected from Spitzer/IRAC…

This work aims to understand which midplane conditions are probed by the DCO$^+$ emission in the disk around the Herbig Ae star HD 169142. We explore the sensitivity of the DCO$^+$ formation pathways to the gas temperature and the CO…

The results of a spectral survey of the region of massive star formation DR21OH in the 4-mm wavelength range are presented. Sixty-nine molecules and their isotopologues have been detected, ranging from simple diatomic or triatomic species…

Astrophysics of Galaxies · Physics 2024-01-31 S. V. Kalenskii , E. A. Mikheeva

Deuterated molecules are a useful diagnostic tool to probe the evolution and the kinematics in the earliest stages of star formation. Due to the low temperatures and high densities in the centre of pre-stellar cores, the deuterium fraction…

Astrophysics of Galaxies · Physics 2026-01-23 K. Giers , S. Spezzano , Y. Lin , P. Caselli , O. Sipilä

Aims. To follow the species chemistry arising in diverse sources of the Galaxy with Herschel. Methods. SPIRE FTS sparse sampled maps of the Orion bar & compact HII regions G29.96-0.02 and G32.80+0.19 have been analyzed. Results. Beyond the…

We report the first detection in space of the two doubly deuterated isotopologues of methyl acetylene. The species CHD2CCH and CH2DCCD were identified in the dense core L483 through nine and eight, respectively, rotational lines in the…

Astrophysics of Galaxies · Physics 2021-06-02 M. Agundez , E. Roueff , C. Cabezas , J. Cernicharo , N. Marcelino

We utilize state-of-the-art 3D hydrodynamical and classical 1D stellar model atmospheres to study the influence of convection on the formation properties of various atomic and molecular spectral lines in the atmospheres of four red giant…

Solar and Stellar Astrophysics · Physics 2013-10-30 V. Dobrovolskas , A. Kučinskas , M. Steffen , H. -G. Ludwig , D. Prakapavičius , J. Klevas , E. Caffau , P. Bonifacio

We present new constraints on gas-phase C, N, and O abundances in the molecular layer of the IM Lup protoplanetary disk. Building on previous physical and chemical modeling of this disk, we use new ALMA observations of C$_2$H to constrain…

Solar and Stellar Astrophysics · Physics 2018-10-17 L. Ilsedore Cleeves , Karin I. Oberg , David J. Wilner , Jane Huang , Ryan A. Loomis , Sean M. Andrews , V. V. Guzman

We report the discovery of four field methane (T-type) brown dwarfs using 2MASS survey data. One additional methane dwarf, previously discovered by SDSS, was also identified. Near-infrared spectra clearly show the 1.6 and 2.2 um CH4…

We present new high contrast imaging of 8 L/T transition brown dwarfs using the NIRC2 camera on the Keck II telescope. One of our targets, the T3.5 dwarf 2MASS J08381155 + 1511155, was resolved into a hierarchal triple with projected…

Solar and Stellar Astrophysics · Physics 2015-06-17 Jacqueline Radigan , Ray Jayawardhana , David Lafrenière , Trent J. Dupuy , Michael C. Liu , Alexander Scholz

We present near-infrared spectra for a sample of T dwarfs, including eleven new discoveries made using the Two Micron All Sky Survey. These objects are distinguished from warmer (L-type) brown dwarfs by the presence of methane absorption…