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Observations of interstellar gas-phase and solid-state species in the 2.4-200 micron range obtained with the spectrometers on board the Infrared Space Observatory are reviewed. Lines and bands due to ices, polycyclic aromatic hydrocarbons,…

Astrophysics · Physics 2009-11-10 Ewine F. van Dishoeck

We report on initial results of our Spitzer Cycle 2 program to observe the young massive star R Mon and its associated HH 39 Herbig-Haro object in the mid-infrared. Our program used all instruments on-board Spitzer to obtain deep images…

Astrophysics · Physics 2007-05-23 M. Audard , S. Skinner , M. Guedel , T. Lanz , F. Paerels , H. Arce

Extragalactic sources from the IRAS Faint Source Catalog (FSC) which have the optically faintest magnitudes (E > 18) were selected by spatial coincidence with a source in the FIRST radio survey, and 28 of these sources have been observed…

Astrophysics · Physics 2015-09-08 Lusine Sargsyan , Areg Mickaelian , Daniel Weedman , James Houck

We present a low-resolution (R = 90), 5.5-38 micron spectral sequence of a sample of M, L, and T dwarfs obtained with the Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope. The spectra exhibit prominent absorption bands of…

Mid-infrared (MIR) quasar spectra exhibit a suite of emission features including high ionization coronal lines from the narrow line region (NLR) illuminated by the ionizing continuum, and hot dust features from grains, as well as polycyclic…

Astrophysics of Galaxies · Physics 2015-06-18 Allison R. Hill , S. C. Gallagher , R. P. Deo , E. Peeters , Gordon T. Richards

Spitzer IRAC and MIPS images of the Trifid Nebula (M20) reveal its spectacular appearance in infrared light, highlighting the nebula's special evolutionary stage. The images feature recently-formed massive protostars and numerous young…

Astrophysics · Physics 2009-11-11 J. Rho , W. T. Reach , B. Lefloch , G. Fazio

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 low-mass star formation. The target has a serendipitous association with a B-type…

Astrophysics of Galaxies · Physics 2022-08-03 E. Kosmaczewski , Ł. Stawarz , W. R. M. Rocha , S. S. Shenoy , A. Karska

We examine 14 hot white dwarfs for signs of infrared excess using the Spitzer Space Telescope. Twelve of the objects are massive white dwarfs which have been suggested to be the result of binary mergers. The remaining two objects are…

Astrophysics · Physics 2008-11-26 Brad M. S. Hansen , Shri Kulkarni , Sloane Wiktorowicz

We present the initial results from the Spitzer Survey of the Small Magellanic Cloud (S3MC), which imaged the star-forming body of the Small Magellanic Cloud (SMC) in all seven MIPS and IRAC wavebands. We find that the F_8/F_24 ratio (an…

We present results on low-resolution mid-infrared (MIR) spectra of 70 infrared-luminous galaxies obtained with the Infrared Spectrograph (IRS) onboard Spitzer. We selected sources from the European Large Area Infrared Survey (ELAIS) with…

We present a study of the stellar and circumstellar properties of Class I sources using low-resolution (R~1000) near-infrared K- and L-band spectroscopy. We measure prominent spectral lines and features in 8 objects and use fits to standard…

Solar and Stellar Astrophysics · Physics 2009-11-13 L. Prato , K. E. Lockhart , Christopher M. Johns-Krull , John T. Rayner

We present mid-infrared observations for a sample of 16 O-type stars. The data were acquired with the NASA Spitzer Space Telescope, using the IRS instrument at moderate resolution (R $\sim$ 600), covering the range $\sim 10-37$ microns. Our…

Solar and Stellar Astrophysics · Physics 2017-07-26 Wagner L. F. Marcolino , Jean-Claude Bouret , Thierry Lanz , Donavan S. Maia , Marc Audard

High-quality K-band spectra of strongly reddened point sources, deeply embedded in (ultra-) compact HII regions, have revealed a population of 20 young massive stars showing no photospheric absorption lines, but sometimes strong Br-gamma…

Astrophysics · Physics 2009-11-11 A. Bik , L. Kaper , L. B. F. M. Waters

We present HST/NICMOS observations with 0.1" (15 AU) resolution of six young stellar objects in the Taurus star-formation region. The targets of our survey are three Class I IRAS sources (IRAS 04016+2610, IRAS 04248+2612, and IRAS…

We present ultraviolet, optical, near-infrared, Spitzer mid-infrared, and radio images of 14 radio-selected objects in M 33. These objects are thought to represent the youngest phase of star cluster formation. We have detected the majority…

Infra-Red(IR) astronomical databases, namely, IRAS, 2MASS, WISE, and Spitzer, are used to analyze photometric data of 126 carbon stars whose spectra are visible in the First Byurakan Survey low-resolution spectral plates. Among these, six…

Solar and Stellar Astrophysics · Physics 2017-04-19 K. S. Gigoyan , A. Sarkissian , C. Rossi , D. Russeil , G. Kostandyan , M. Calabresi , F. Zamkotsian , M. Meftah

Context. Episodic accretion in young stellar objects (YSOs) is thought to play a critical role in addressing the "luminosity problem" associated with star formation. However, optical surveys tend to bias against sources that are heavily…

Solar and Stellar Astrophysics · Physics 2026-04-22 Jiaxun Li , Tinggui Wang , Zheyu Lin

We conducted an infrared search for faint companions around 351 young stellar objects in the rho Ophiucus molecular cloud and the Serpens molecular cloud. Nine objects in the Spitzer/IRAC archival images were identified as young stellar…

Solar and Stellar Astrophysics · Physics 2015-05-28 Chiaki Shirono , Yoichi Itoh , Yumiko Oasa

Jets and outflows are associated with young stellar objects across the stellar mass spectrum, from brown dwarf protostars to massive, Ae/Be stars. Frequently, the jet morphology is spatially discontinuous because of the temporal variability…

Solar and Stellar Astrophysics · Physics 2021-04-14 Rosario López , Angels Riera , Robert Estalella , Gabriel Gómez

We present new Spitzer Space Telescope observations of the region NGC 2467, and use these observations to determine how the environment of an HII region affects the process of star formation. Our observations comprise IRAC (3.6, 4.5, 5.8,…

Astrophysics · Physics 2009-07-22 Keely D. Snider , J. Jeff Hester , Steven J. Desch , Kevin R. Healy , Jon Bally