Search Results - "Karska, A."
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Multiwavelength Study of Dark Globule DC 314.8–5.1: Point-source Identification and Diffuse Emission Characterization
Published in The Astrophysical journal (01-12-2023)“…Abstract We present an analysis of multiwavelength observations of the dark globule DC 314.8–5.1, using data from the Gaia optical, Two Micron All Star…”
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Environments of red nuggets at z ∼ 0.7 from the VIPERS survey
Published in Monthly notices of the Royal Astronomical Society (08-06-2023)“…ABSTRACT Red ultra-compact massive galaxies, called red nuggets were formed at high redshifts (z ∼ 2–3). Survivors of red nuggets, known as relics, observed at…”
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3
Spectroscopic Diagnostics of the Mid-infrared Features of the Dark Globule DC 314.8–5.1 with the Spitzer Space Telescope
Published in The Astrophysical journal (01-08-2022)“…Abstract We present an analysis of the mid-infrared spectra, obtained from the Spitzer Space Telescope, of the dark globule DC 314.8–5.1, which is at the onset…”
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4
OGHReS: star formation in the outer galaxy (ℓ = 250°–280°)
Published in Monthly notices of the Royal Astronomical Society (01-03-2024)“…ABSTRACT We have used data from the Outer Galaxy High-Resolution Survey (OGHReS) to refine the velocities, distances, and physical properties of a large sample…”
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5
The H2O Spectrum of the Massive Protostar AFGL 2136 IRS 1 from 2 to 13 μm at High Resolution: Probing the Circumstellar Disk
Published in The Astrophysical journal (01-05-2020)“…We have observed the massive protostar AFGL 2136 IRS 1 in multiple wavelength windows in the near- to mid-infrared at high (∼3 km s−1) spectral resolution…”
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An ALMA survey of the SCUBA-2 cosmology legacy survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman-break galaxies
Published in Monthly notices of the Royal Astronomical Society (2020)“…ABSTRACT We analyse 870 $\mu$m Atacama Large Millimetre Array (ALMA) dust continuum detections of 41 canonically selected $z$ ≃ 3 Lyman-break galaxies (LBGs),…”
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Origins Space Telescope: From First Light to Life
Published in Experimental astronomy (01-06-2021)“…The Origins Space Telescope (Origins) is one of four science and technology definition studies selected by National Aeronautics and Space Administration (NASA)…”
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Ubv(Ri)C Photometry of the Contact W Uma Binary Bd + 14∘5016
Published in Astrophysics and space science (01-01-2005)“…New UBV(RI)C observations and radial velocities of the W UMa-type system BD + 14[compfn]5016 were collected. Changes of the properties of a hot spot, located…”
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9
The H2O Spectrum of the Massive Protostar AFGL 2136 IRS 1 from 2 to 13 m at High Resolution: Probing the Circumstellar Disk
Published in The Astrophysical journal (12-05-2020)“…We have observed the massive protostar AFGL 2136 IRS 1 in multiple wavelength windows in the near- to mid-infrared at high (∼3 km s−1) spectral resolution…”
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Journal Article -
10
The H 2 O Spectrum of the Massive Protostar AFGL 2136 IRS 1 from 2 to 13 μm at High Resolution: Probing the Circumstellar Disk
Published in The Astrophysical journal (01-05-2020)“…Abstract We have observed the massive protostar AFGL 2136 IRS 1 in multiple wavelength windows in the near- to mid-infrared at high (∼3 km s −1 ) spectral…”
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Journal Article -
11
Water in Star-forming Regions with the Herschel Space Observatory (WISH). I. Overview of Key Program and First Results
Published in Publications of the Astronomical Society of the Pacific (2011)“…Water In Star-forming regions with Herschel (WISH) is a key program on the Herschel Space Observatory designed to probe the physical and chemical structures of…”
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12
Origins space telescope: from first light to life
Published in Experimental astronomy (01-06-2021)“…Abstract The Origins Space Telescope (Origins) is one of four science and technology definition studies selected by the National Aeronautics and Space…”
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13
Effects of stellar feedback on cores in STARFORGE
Published 09-09-2024“…A&A 690, A345 (2024) Stars form in dense cores within molecular clouds and newly formed stars influence their natal environments. How stellar feedback impacts…”
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14
Unsupervised classification reveals new evolutionary pathways
Published 21-11-2022“…While we already seem to have a general scenario of the evolution of different types of galaxies, a complete and satisfactory understanding of the processes…”
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15
Multiwavelength Study of Dark Globule DC 314.8-5.1: Point Source Identification and Diffuse Emission Characterization
Published 06-09-2022“…We present an analysis of multi-wavelength observations of the dark globule DC\,314.8--5.1, using data from the Gaia optical, 2MASS near-infrared, and WISE…”
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Journal Article -
16
Environments of red nuggets at z~0.7 from the VIPERS survey
Published 12-06-2023“…Red ultra-compact massive galaxies, called red nuggets were formed at high redshifts ($\rm{z\sim2-3}$). Survivors of red nuggets, known as relics, observed at…”
Get full text
Journal Article -
17
Spectroscopic Diagnostics of the Mid-Infrared Features of the Dark Globule, DC 314.8-5.1, with the Spitzer Space Telescope
Published 17-06-2022“…We present an analysis of the mid-infrared spectra, obtained from the Spitzer Space Telescope, of the dark globule, DC 314.8--5.1, which is at the onset of…”
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Journal Article -
18
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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Journal Article -
19
Ubv(Ri)C Photometry of the Contact W Uma Binary Bd + 145016
Published in Astrophysics and space science (01-04-2005)“…New UBV(RI)^sub C^ observations and radial velocities of the W UMa-type system BD + 14^sup ^5016 were collected. Changes of the properties of a hot spot,…”
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Journal Article -
20
OGHReS: Star formation in the Outer Galaxy ($\ell = 250^\circ$-$280^\circ$)
Published 01-01-2024“…We have used data from the Outer Galaxy High-Resolution Survey (OGHReS) to refine the velocities, distances, and physical properties of a large sample of 3584…”
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