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We present new narrow-band near-infrared images together with K band spectra of highly collimated bipolar jets close to the IRAS 05487+0255 source. The jets are located at 50" West of the Herbig-Haro 110 outflow. The jets are not visible at…

天体物理学 · 物理学 2009-10-30 P. Garnavich , A. Noriega-Crespo , A. Raga , K. H. Bohm

The central area (40"x40") of the bipolar nebula S106 was mapped in the OI line at 63.2 micron with high angular (6") and spectral resolution, using GREAT on board SOFIA. The OI emission distribution is compared to the CO 16-15, CII 158…

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 have observed emission lines of [S IV] 10.51, H(7-6) 12.37, [Ne II] 12.81, [Ne III] 15.56, and [S III] 18.71 um in a number of extragalactic H II regions with the Spitzer Space Telescope. A previous paper presented our data and analysis…

We produce simulations of emission of the atomic CII line in large sky fields in order to determine the current prospects for mapping this line during the high redshift Epoch of Reionization. We estimate the CII line intensity, redshift…

星系天体物理 · 物理学 2015-05-22 Marta B. Silva , Mário G. santos , Asantha Cooray , Yan Gong

We observed the neutron star (NS) ultra-compact X-ray binary 4U0614+091 quasi-simultaneously in the radio band (VLA), mid-IR/IR (Spitzer/MIPS and IRAC), near-IR/optical (SMARTS), optical-UV (Swift/UVOT), soft and hard X-rays (Swift/XRT and…

高能天体物理现象 · 物理学 2014-11-20 S. Migliari , J. A. Tomsick , J. C. A. Miller-Jones , S. Heinz , R. I. Hynes , R. P. Fender , E. Gallo , P. G. Jonker , T. J. Maccarone

Fine-structure mid-infrared emission lines with critical densities in the regime 10^4 to 10^6 cm^-3 can be employed to probe the outflow from Wolf-Rayet stars at radii of \sim 10^15 cm. Narrow-band mid-infrared imaging and spectroscopy of…

太阳与恒星天体物理 · 物理学 2015-06-11 P. F. Roche , M. D. Colling , M. J. Barlow

The physical conditions in the inner narrow line region (NLR) of the Seyfert 2 galaxy NGC 1068 are examined using HST/STIS ultraviolet and optical spectra and photoionization models. 1) The emission-line gas in the blueshifted northeast…

天体物理学 · 物理学 2009-10-31 Steven B. Kraemer , D. Michael Crenshaw

We have obtained the first high spatial (0.05'') and spectral (R~35000) resolution 2 micron spectrum of the T Tau S tight binary system using adaptive optics on the Keck II telescope. We have also obtained the first 3.8 and 4.7 micron…

天体物理学 · 物理学 2009-11-11 G. Duchene , A. M. Ghez , C. McCabe , C. Ceccarelli

We present results on the properties of neon emission in $z\sim2$ star-forming galaxies drawn from the MOSFIRE Deep Evolution Field (MOSDEF) survey. Doubly-ionized neon ([NeIII]3869) is detected at $\geq3\sigma$ in 61 galaxies, representing…

We have obtained high resolution spectra (R = 25000) of an A star over varying airmass to determine the effectiveness of telluric removal in the limit of high signal to noise. The near infra-red line HeI at 2.058 microns, which is a…

天体物理学 · 物理学 2015-06-24 M. A. Kenworthy , M. M. Hanson

Jets from young stars represent one of the most striking signposts of star formation. The phenomenon has been researched for over two decades and there is now general agreement that such jets are generated as a by-product of accretion; most…

天体物理学 · 物理学 2007-05-23 Tom Ray , Catherine Dougados , Francesca Bacciotti , Jochen Eisloeffel , Antonio Chrysostomou

Context: Microquasars are accreting Galactic sources that are also observed to launch relativistic jets. A key signature of the ejection is non-thermal radio emission. The level of this jet component at high frequencies is still poorly…

高能天体物理现象 · 物理学 2015-05-27 Sylvain Chaty , Guillaume Dubus , Anand Raichoor

We present results from a spectroscopic Spitzer and Herschel mid-to-far-infrared study of the circumbinary disk orbiting the evolved (age ~12-23 Myr) close binary T Tauri system V4046 Sgr. Spitzer IRS spectra show emission lines of [Ne II],…

Interstellar reddening corrections are necessary to reconstruct the intrinsic spectral energy distributions (SEDs) of accreting protostellar systems. The stellar SED determines the heating and chemical processes that can occur in…

At early stages of stellar evolution young stars show powerful jets and/or outflows that interact with protoplanetary discs and their surroundings. Despite the scarce knowledge about the interaction of jets and/or outflows with discs,…

太阳与恒星天体物理 · 物理学 2017-07-26 M. Alonso-Martinez , P. Riviere-Marichalar , G. Meeus , I. Kamp , M. Fang , L. Podio , W. R. F. Dent , C. Eiroa

We report sensitive Spitzer IRS spectroscopy in the 10-20 micron region of TW Hya, a nearby T Tauri star. The unusual spectral energy distribution of the source, that of a transition object, indicates that the circumstellar disk in the…

太阳与恒星天体物理 · 物理学 2015-05-18 Joan R. Najita , John S. Carr , Stephen E. Strom , Dan M. Watson , Ilaria Pascucci , David Hollenbach , Uma Gorti , Luke Keller

We present survey results which suggest rotation signatures at the base of T-Tauri jets. Observations were conducted with the Hubble Space Telescope Imaging Spectrograph at optical and near ultraviolet wavelengths (NUV). Results are…

天体物理学 · 物理学 2011-02-11 Deirdre Coffey , Francesca Bacciotti , Thomas P. Ray , Jochen Eislöffel , Jens Woitas

We present new ISO-SWS data for a sample of 27 starburst galaxies, and with these data examine the issues of formation and evolution of the most massive stars in starburst galaxies. Using starburst models which incorporate time evolution,…

天体物理学 · 物理学 2011-05-05 M. D. Thornley , N. M. Forster-Schreiber , D. Lutz , R. Genzel , H. W. W. Spoon , D. Kunze , A. Sternberg

We present spatially resolved emission diagnostics for eight $z\sim0.9$ galaxies that demonstrate extended low ionization emission-line regions (LIERs) over kpc scales. Eight candidates are selected based on their spatial extent and…