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Related papers: Spitzer Discovery of Very Low Luminosity Objects

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CH4 is proposed to be the starting point of a rich organic chemistry. Solid CH4 abundances have previously been determined mostly toward high mass star forming regions. Spitzer/IRS now provides a unique opportunity to probe solid CH4 toward…

We have observed 14 nearby (z<0.16) Ultraluminous Infrared Galaxies (ULIRGs) with Spitzer at 3.6-24 microns. The underlying host galaxies are well-detected, in addition to the luminous nuclear cores. While the spatial resolution of Spitzer…

Astrophysics · Physics 2007-05-23 J. A. Surace , Z. Wang , S. Willner , H. Smith , J. Pipher , W. Forrest , G. Fazio

(abbreviated) We report detection with the Spitzer Space Telescope of cool dust surrounding solar type stars. The observations were performed as part of the Legacy Science Program, ``Formation and Evolution of Planetary Systems'' (FEPS).…

We examine the infrared properties of five low surface brightness galaxies (LSBGs) and compare them with related but higher surface brightness galaxies, using Spitzer Space Telescope images and spectra. All the LSBGs are detected in the 3.6…

Combining the relative vicinity of the Local Group spiral galaxy M33 with the Spitzer images, we investigate the properties of infrared (IR) emission sites and assess the reliability of the IR emission as a star formation tracer. We…

Astrophysics · Physics 2007-12-05 S. Verley , L. K. Hunt , E. Corbelli , C. Giovanardi

We have retrieved Spitzer archive data of pre-stellar cores taken with the Multiband Imaging Photometer for Spitzer (MIPS) at a wavelength of 160 um. Seventeen images, containing eighteen cores, were constructed. Flux densities were…

Astrophysics · Physics 2008-11-26 J. M. Kirk , D. Ward-Thompson , P. Andre

We present a search for outflows towards 51 submillimetre cores in Perseus. With consistently derived outflow properties from a large homogeneous dataset within one molecular cloud we can investigate further the mass dependence and time…

Astrophysics · Physics 2009-11-13 J. Hatchell , G. A. Fuller , J. S. Richer

The Cold Dark Matter (CDM) model for galaxy formation predicts that a significant fraction of mass in the dark matter haloes that surround L L* galaxies is bound in substructures of mass 1E4-1E7Msun. The number of observable baryonic…

Astrophysics · Physics 2009-11-07 Leonidas A. Moustakas , R. Benton Metcalf

Dark matter in the Universe consisting of macroscopic objects such as primordial black holes may cause gravitational lensing of distant objects. The magnification associated with lensing will lead to additional scatter in the received flux…

Astrophysics · Physics 2009-11-06 Elspeth M. Minty , Alan F. Heavens , Michael R. S. Hawkins

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 Spitzer high-resolution spectra of off-nuclear regions in the central cluster galaxies NGC 1275 and NGC 4696 in the Perseus and Centaurus clusters, respectively. Both objects are surrounded by extensive optical emission-line…

Astrophysics · Physics 2009-11-13 R. Johnstone , N. Hatch , G. Ferland , A. Fabian , C. Crawford , R. Wilman

A powerful way to observe directly the solid state inventory of dense molecular clouds is by infrared spectroscopy of background stars. We present Spitzer/IRS 5-20 micron spectra of ices toward stars behind the Serpens and Taurus molecular…

The SOLIS (Seeds Of Life In Space) IRAM/NOEMA Large Program aims at studying a set of crucial complex organic molecules in a sample of sources, with well-known physical structure, covering the various phases of Solar-type star formation.…

Water is an important molecule in the chemical and thermal balance of dense molecular gas, but knowing its history through-out the various stages of the star formation is a fundamental problem. Its molecular deuteration provides us with a…

Solar and Stellar Astrophysics · Physics 2015-12-16 David Quénard , Vianney Taquet , Charlotte Vastel , Paola Caselli , Cecilia Ceccarelli

The nearly continuous light curves with micromagnitude precision provided by the space mission Kepler are revolutionising our view of pulsating stars. They have revealed a vast sea of low-amplitude pulsation modes that were undetectable…

Physical conditions that could render a core starless(in the local Universe) is the subject of investigation in this work. To this end we studied the evolution of four starless cores, B68, L694-2, L1517B, L1689, and L1521F, a VeLLO. The…

Astrophysics of Galaxies · Physics 2016-08-24 S. Anathpindika

We present K-band polarimetric images of several massive young stellar objects at resolutions $\sim$ 0.1-0.5 arcsec. The polarization vectors around these sources are nearly centro-symmetric, indicating they are dominating the illumination…

Astrophysics · Physics 2009-11-13 Zhibo Jiang , Motohide Tamura , Melvin G. Hoare , Yongqiang Yao , Miki Ishii , Min Fang , Ji Yang

The first observations of the infrared spectrum of the LMC planetary nebula SMP83 as observed by the recently launched Spitzer Space Telescope are presented. The high resolution R~600 spectrum shows strong emission lines but no significant…

Astrophysics · Physics 2007-05-23 J. Bernard-Salas , J. R. Houck , P. W. Morris , G. C. Sloan , S. R. Pottasch , D. J. Barry

Low-mass dark matter (DM) subhalos are pivotal in understanding the small-scale structure of the universe, thereby offering a sensitive method to discriminate between different cosmological models. In this study, we estimate the local…

High Energy Physics - Phenomenology · Physics 2025-04-21 Xiuyuan Zhang , Lina Necib , Denis Erkal

We report on the first attempts at searching for CO in red low surface brightness galaxies, and the first detection of molecular gas in a low surface brightness (mu_B(0)_{obs} > 23 mag arcsec^{-2}) galaxy. Using the IRAM 30m telescope,…

Astrophysics · Physics 2009-10-31 K. O'Neil , P. Hofner , E. Schinnerer