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We present new infrared data from a survey for embedded protostellar jets in the Orion A cloud. This survey makes use of the S(1) v = 1-0 line of molecular hydrogen at lambda = 2.12 mum to search for infrared jets deep inside the cloud and…

Astrophysics · Physics 2007-05-23 Thomas Stanke , Mark J. McCaughrean , Hans Zinnecker

We present new observational data for IRAS 09371+1212, the Frosty Leo Nebula, in the form of infrared spectra from 2.2-2.5 microns which reveal photopheric bands of CO. The ^12CO/^13CO band ratio determined is similar to those exhibited by…

Astrophysics · Physics 2007-05-23 Tyler Bourke , A. R. Hyland , Garry Robinson , Kevin Luhman

Observations of outflows associated with pre-main-sequence stars reveal details about morphology, binarity and evolutionary states of young stellar objects. We present molecular line data from the Berkeley-Illinois-Maryland Association…

Astrophysics · Physics 2009-11-13 Brenda C. Matthews , James R. Graham , Marshall D. Perrin , Paul Kalas

Context: Planetary nebulae (PNe) are excellent tracers of stellar populations with low surface brightness, and therefore provide a powerful method to detect and explore the rich system of substructures discovered around the main spiral…

Astrophysics of Galaxies · Physics 2018-04-18 R. Galera-Rosillo , R. L. M. Corradi , A. Mampaso

We have carried out mid-infrared spectroscopy of seven Galactic proto-planetary nebulae (PPNs) using the Spitzer Space Telescope. They were observed from 10-36 microns at relatively high spectral resolution, R~600. The sample was chosen…

Solar and Stellar Astrophysics · Physics 2011-02-11 Bruce J. Hrivnak , Kevin Volk , Sun Kwok

NGC 6369 is a double-shell planetary nebula (PN) consisting of a bright annular inner shell with faint bipolar extensions and a filamentary envelope. We have used ground- and space-based narrow-band optical and near-IR images, broad-band…

Solar and Stellar Astrophysics · Physics 2015-06-03 Gerardo Ramos-Larios , Martin A. Guerrero , Roberto Vazquez , J. P. Phillips

We present a survey for extended 2.2 $\mu$m emission in 20 new visual reflection nebulae, illuminated by stars with temperatures of 3,600 --- 33,000 K. We detect extended 2.2 $\mu$m emission in 13 new nebulae, illuminated by stars with…

Astrophysics · Physics 2009-10-28 K. Sellgren , M. W. Werner , L. J. Allamandola

We report the discovery of a dozen Herbig-Haro jets illuminated by the Lyman continuum and/or softer far-ultraviolet radiation fields of nearby high mass stars. Five irradiated outflows lie in the outer parts of the Orion Nebula and seven…

Astrophysics · Physics 2009-10-31 John Bally , Bo Reipurth

[Abridged] We present Far Ultraviolet Spectroscopic Explorer (FUSE) observations of the young, compact planetary nebula (PN) SwSt 1 along the line of sight to its central star HD 167362. We detect circumstellar absorption lines from several…

Astrophysics · Physics 2009-11-10 N. C. Sterling , H. L. Dinerstein , C. W. Bowers , S. Redfield

We describe an object in the Hubble Deep Field North with very unusual near-infrared properties. It is readily visible in Hubble Space Telescope NICMOS images at 1.6um and from the ground at 2.2um, but is undetected (with signal-to-noise <~…

The core of the nebula surrounding Eta Carinae has been observed with the VLT Adaptive Optics system NACO and with the interferometer VLTI/MIDI to constrain spatially and spectrally the warm dusty environment and the central object. In…

We have obtained narrow-band images and high-resolution spectra of the planetary nebulae NGC 6337, He 2-186, and K 4-47, with the aim of investigating the relation between their main morphological components and several low-ionization…

One of the major challenges to identification of the 3.3, 6.2, 7.7, 8.6, and 11.3um interstellar IR emission bands with polycyclic aromatic hydrocarbon (PAH) molecules has been the recent detection of these bands in regions with little UV…

Astrophysics · Physics 2009-11-07 Aigen Li , B. T. Draine

A large, faint nebula was unexpectedly discovered near M31 using narrowband [O III] images. Its apparent size and the lack of a clear counterpart at other wavelengths make it unique and challenging to explain. We aim to determine whether…

We describe multi-wavelength (8--20 micron), diffraction-limited, mid-infrared images of the OMC-1 cloud core in Orion, covering an approximately two arcminute area around the Trapezium and BN/KL regions. We have detected mid-infrared…

Astrophysics · Physics 2007-05-23 L. K. Deutsch , M. Kassis , N. Smith , J. L. Hora , H. M. Butner , W. F. Hoffmann , G. G. Fazio , A. Dayal

IRAS18197-1118 is a stellar-like object that has been classified as a planetary nebula from its radio continuum emission and high [SIII]9532 to Paschen9 line intensity ratio, as derived from direct images. We present intermediate- and…

Solar and Stellar Astrophysics · Physics 2015-06-19 L. F. Miranda , L. F. Rodriguez , C. B. Pereira , R. Vazquez

We investigate the polycyclic aromatic hydrocarbon features in the young Galactic planetary nebula PN G095.2+00.7 based on mid-infrared observations. The near- to mid-infrared spectra obtained with the AKARI/IRC and the Spitzer/IRS show the…

Solar and Stellar Astrophysics · Physics 2012-11-13 Ryou Ohsawa , Takashi Onaka , Itsuki Sakon , Tamami I. Mori , Takashi Miyata , Kentaro Asano , Mikako Matsuura , Hidehiro Kaneda

In order to look for signs of on-going planet formation in young disks, we carried out the first J-band polarized emission imaging of the Herbig Ae/Be stars HD 150193, HD 163296, and HD 169142 using the Gemini Planet Imager (GPI), along…

We have conducted the first systematic study of Herbig Ae/Be stars using the technique of long baseline stellar interferometry in the near-infrared. The principal result of this paper is that the IOTA interferometer resolves the source of…

Astrophysics · Physics 2009-10-31 Rafael Millan-Gabet , F. Peter Schloerb , Wesley A. Traub

Sh 2-174 is believed to be either a planetary nebula (PN) or ionized, ambient interstellar medium (ISM). We present in this paper 1420 MHz polarization, 1420 MHz total intensity (Stokes-I), and neutral hydrogen (HI) images of the region…

Astrophysics of Galaxies · Physics 2015-06-23 R. R. Ransom , R. Kothes , J. Geisbuesch , W. Reich , T. L. Landecker