Search Results - "Yıldız, U. A."
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Striations in the Taurus molecular cloud: Kelvin–Helmholtz instability or MHD waves?
Published in Monthly notices of the Royal Astronomical Society (01-10-2016)“…The origin of striations aligned along the local magnetic field direction in the translucent envelope of the Taurus molecular cloud is examined with new…”
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2
The APEX Large CO Heterodyne Orion Legacy Survey (ALCOHOLS). I. Survey overview
Published 03-01-2022“…A&A 658, A178 (2022) The Orion molecular cloud complex harbours the nearest GMCs and site of high-mass star formation. Its YSO populations are thoroughly…”
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Classifying the embedded young stellar population in Perseus and Taurus & the LOMASS database
Published 10-11-2015“…A&A 586, A44 (2016) Context. The classification of young stellar objects (YSOs) is typically done using the infrared spectral slope or bolometric temperature,…”
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Outflows, infall and evolution of a sample of embedded low-mass protostars. The William Herschel Line Legacy (WILL) survey
Published 19-01-2017“…[Abridged] We present spectroscopic observations in H$_{2}$O, CO and related species with \textit{Herschel} HIFI and PACS, as well as ground-based follow-up…”
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Observations and modelling of CO and [CI] in disks. First detections of [CI] and constraints on the carbon abundance
Published 07-01-2016“…A&A 588, A108 (2016) The gas-solid budget of carbon in protoplanetary disks is related to the composition of the cores and atmospheres of the planets forming…”
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High-pressure, low-abundance water in bipolar outflows. Results from a Herschel-WISH survey
Published 22-01-2013“…(Abridged) We present a survey of the water emission in a sample of more than 20 outflows from low mass young stellar objects with the goal of characterizing…”
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Multi-line detection of O2 toward rho Oph A
Published 25-02-2012“…Models of pure gas-phase chemistry in well-shielded regions of molecular clouds predict relatively high levels of molecular oxygen, O2, and water, H2O…”
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Water in massive star-forming regions: HIFI observations of W3 IRS5
Published 28-09-2010“…We present Herschel observations of the water molecule in the massive star-forming region W3 IRS5. The o-H17O 110-101, p-H18O 111-000, p-H2O 22 202-111, p-H2O…”
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Herschel-HIFI observations of high-J CO lines in the NGC 1333 low-mass star-forming region
Published 18-08-2010“…A&A HIFI Special Issue, 2010 Herschel-HIFI observations of high-J lines (up to J_u=10) of 12CO, 13CO and C18O are presented toward three deeply embedded…”
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HERSCHEL-HIFI spectroscopy of the intermediate mass protostar NGC7129 FIRS 2
Published 06-08-2010“…HERSCHEL-HIFI observations of water from the intermediate mass protostar NGC7129 FIRS 2 provide a powerful diagnostic of the physical conditions in this star…”
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Variations in H2O+/H2O ratios toward massive star-forming regions
Published 26-07-2010“…Early results from the Herschel Space Observatory revealed the water cation H2O+ to be an abundant ingredient of the interstellar medium. Here we present new…”
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Herschel-HIFI detections of hydrides towards AFGL 2591 (Envelope emission versus tenuous cloud absorption)
Published 20-07-2010“…The Heterodyne Instrument for the Far Infrared (HIFI) onboard the Herschel Space Observatory allows the first observations of light diatomic molecules at high…”
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13
Water in low-mass star-forming regions with Herschel: HIFI spectroscopy of NGC1333
Published 18-07-2010“…'Water In Star-forming regions with Herschel' (WISH) is a key programme dedicated to studying the role of water and related species during the star-formation…”
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Dust, Ice and Gas in Time (DIGIT) Herschel program first results: A full PACS-SED scan of the gas line emission in protostar DK Cha
Published 14-05-2010“…DK Cha is an intermediate-mass star in transition from an embedded configuration to a star plus disk stage. We aim to study the composition and energetics of…”
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15
Water in Star-forming Regions with theHerschel Space Observatory(WISH). I. Overview of Key Program and First Results
Published in Publications of the Astronomical Society of the Pacific (11-02-2011)“…Water In Star-forming regions withHerschel(WISH) is a key program on theHerschel Space Observatorydesigned to probe the physical and chemical structures of…”
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Striations in the Taurus molecular cloud: Kelvin-Helmholtz instability or MHD waves?
Published 28-06-2016“…The origin of striations aligned along the local magnetic field direction in the translucent envelope of the Taurus molecular cloud is examined with new…”
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Journal Article -
17
Herschel Measurements of Molecular Oxygen in Orion
Published in The Astrophysical journal (20-08-2011)“…We report observations of three rotational transitions of molecular oxygen (O2) in emission from the H2 Peak 1 position of vibrationally excited molecular…”
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Origin of warm and hot gas emission from low-mass protostars: Herschel-HIFI observations of CO J=16-15. I. Line profiles, physical conditions, and H2O abundance
Published 29-05-2017“…A&A 605, A93 (2017) (Abridged) Through spectrally unresolved observations of high-J CO transitions, Herschel-PACS has revealed large reservoirs of warm (300 K)…”
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HERSCHEL HIFI OBSERVATIONS OF O 2 TOWARD ORION: SPECIAL CONDITIONS FOR SHOCK ENHANCED EMISSION
Published in The Astrophysical journal (01-10-2014)“…We report observations of molecular oxygen (O-2) rotational transitions at 487 GHz, 774 GHz, and 1121 GHz toward Orion Peak A. The O-2 lines at 487 GHz and 774…”
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The hot core towards the intermediate mass protostar NGC7129 FIRS 2: Chemical similarities with Orion KL
Published 19-05-2014“…A&A 568, A65 (2014) NGC 7129 FIRS 2 (hereafter FIRS 2) is an intermediate-mass (2 to 8 Msun) protostar located at a distance of 1250 pc. High spatial…”
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