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IRAS F11119+3257 is a quasar-dominated Ultra-Luminous InfraRed Galaxy, with a partially obscured narrow-line seyfert 1 nucleus. In this paper, we present the NIR spectroscopy of F11119+3257, in which we find unusual Paschen emission lines,…

Astrophysics of Galaxies · Physics 2019-10-14 Xiang Pan , Hongyan Zhou , Wenjuan Liu , Bo Liu , Tuo Ji , Xiheng Shi , Shaohua Zhang , Peng Jiang , Huiyuan Wang , Lei Hao

We present a 350 micron APEX/SABOCA map of IRAS 05399-0121/SMM 1, which is a dense double-core system in Orion B9. We combined these data with our previous LABOCA 870-micron data. The spatial resolution of the new SABOCA image, ~3400 AU, is…

Astrophysics of Galaxies · Physics 2015-06-15 Oskari Miettinen , Stella S. R. Offner

We report interferometric observations of the high-mass star-forming object IRAS 23033+5951. Our observations reveal two massive molecular cloud cores, designated IRAS 23033+5951-MMS1 and IRAS 23033+5951-MMS2. MMS1 has already formed a…

Astrophysics · Physics 2009-11-13 Michael A. Reid , Brenda C. Matthews

We report the discovery of a young, 0.16" binary, 2M2234+4041AB, found as the result of a Keck laser guide star adaptive optics imaging survey of young field ultracool dwarfs. Spatially resolved near-infrared photometry and spectroscopy…

A multi-wavelength investigation of the star forming complex IRAS 20286+4105, located in the Cygnus-X region, is presented here. Near-infrared K-band data is used to revisit the cluster / stellar group identified in previous studies. The…

Solar and Stellar Astrophysics · Physics 2016-11-10 Varsha R , S. R. Das , A. Tej , S. Vig , S. K. Ghosh , D. K. Ojha

Using the 13.7 m telescope of Purple Mountain Observatory (PMO), a survey of J=1-0 lines of CO and its isotopes was carried out towards 98 methanol maser sources in January 2008. Eighty-five sources have infrared counterparts within one…

Solar and Stellar Astrophysics · Physics 2015-06-04 Tie Liu , Yue-Fang Wu , Ke Wang

IRAS 21413+5442 and IRAS 21407+5441 are two massive star forming regions of high luminosity, likely associated with each other. Near-infrared photometry on these two IRAS sources was performed at UKIRT using the UFTI under excellent seeing…

Astrophysics · Physics 2009-11-13 B. G. Anandarao , V. Venkata Raman , S. K. Ghosh , D. K. Ojha , M. S. N. Kumar

The mapping observations of CO $J=2-1$, CO $J=3-2$, $^{13}$CO $J=2-1$ and $^{13}$CO $J=3-2$ lines in the direction of IRAS 22506+5944 have been made. The results show that the cores in the $J=2-1$ transition lines have a similar morphology…

Solar and Stellar Astrophysics · Physics 2010-01-29 Jin-Long Xu , Jun-Jie Wang

The physical conditions of the interstellar medium and stellar components in the regions of the southern Galactic star forming complexes associated with IRAS 10049-5657 and IRAS 10031-5632 have been investigated. These regions have been…

Astrophysics · Physics 2009-11-13 S. Vig , S. K. Ghosh , D. K. Ojha , R. P. Verma

We present observations of the star formation region NGC 7129 taken with the Multiband Imaging Photometer for Spitzer (MIPS). A significant population of sources, likely pre-main sequence members of the young stellar cluster, is revealed…

Rest-frame 0.48-1.1 micron emission line strengths and molecular gas mass (H_2) upper limits for 3 luminous infrared sources - the hyperluminous infrared galaxies IR F09105+4108 (z=0.44), IR F15307+3252 (z=0.93), and the optically-selected…

The Herbig Ae star HD 139614 is a group-Ib object, which featureless SED indicates disk flaring and a possible pre-transitional evolutionary stage. We present mid- and near-IR interferometric results collected with MIDI, AMBER and PIONIER…

The four-image gravitationally lensed quasar QSO 2237+0305 is microlensed by stars in the lens galaxy. The amplitude of microlensing variability can be used to infer the relative size of the quasar as a function of wavelength; this provides…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-11 Eric Agol , Stephanie Gogarten , Varoujan Gorjian , Amy Kimball

We present an analysis of the IRAS 08589-4714 star-forming region. This region harbors candidate young stellar objects identified in the WISE and Herschel images using color index criteria and spectral energy distributions (SEDs). The SEDs…

Solar and Stellar Astrophysics · Physics 2016-09-06 H. P. Saldaño , J. Vásquez , M. Gómez , C. E. Cappa , N. U. Duronea , M. Rubio

We report the detection of strong absorption and weak emission features in the 4--27 micron Spitzer-IRS spectrum of the distant ultraluminous infrared galaxy (ULIRG) IRAS F00183--7111 (z=0.327). The absorption features of CO2 and CO gas,…

Two Galactic star forming regions, one in a very early phase of evolution and another evolved one, associated with the IRAS sources 00338+6312 and 03595+5110 (RAFGL 5111) respectively have been studied in detail. These sources have been…

Astrophysics · Physics 2009-10-31 B. Mookerjea , S. K. Ghosh , A. D. Karnik , T. N. Rengarajan , S. N. Tandon , R. P. Verma

We present Spitzer IRAC and IRS observations of the dark cloud L1287. The mid-infrared (MIR) IRAC images show deeply embedded infrared sources in the vicinity of the FU Orionis objects RNO 1B and RNO 1C suggesting their association with a…

Astrophysics · Physics 2009-01-19 S. P. Quanz , Th. Henning , J. Bouwman , H. Linz , F. Lahuis

UVES spectra of the very young (~10^7 years) peculiar B-type star HR 6000 were analyzed in the near-UV and visual spectral regions (3050-9460 A) with the aim to extend to other spectral ranges the study made previously in the UV using IUE…

Astrophysics · Physics 2009-11-13 F. Castelli , S. Hubrig

We present high resolution optical spectroscopic observations of IRAS 09425-6040, a peculiar, extremely red, C-rich AGB star showing prominent O-rich dust features in its ISO infrared spectrum attributed to crystalline silicates. Our…

Astrophysics · Physics 2009-11-11 D. A. Garcia-Hernandez , C. Abia , A. Manchado , P. Garcia-Lario

The Spitzer-GLIMPSE point source catalog and images have been used to study a sample of 381 massive protostellar candidates. IRAC-Point source photometry was used to analyse colours, magnitudes and spectral indicies of the infrared…

Astrophysics · Physics 2008-02-15 M. S. N. Kumar , J. M. C. Grave