Results 1 to 10 of about 2,045,808 (218)

Discovery of Volatile Gas in the Giant Impact Disk Around the 150 Myr Old HD 23514

open access: yesThe Astrophysical Journal Letters
We report the discovery of CO _2 gas emission around HD 23514, an F5V star in the ∼150 Myr old Pleiades cluster, hosting one of the rare giant-impact disks with unique mineralogy dominated by silica dust. We show that the dust feature remains stable over
Kate Y. L. Su   +10 more
doaj   +1 more source

The 12CO gas structures of protoplanetary disks in the Upper Scorpius region

open access: yesAstronomy & Astrophysics
We present measurements of key protoplanetary disk properties inferred from parametric models of ALMA 12CO spectral line visibilities. We derived gas-disk radii, integrated fluxes, optically thick emission layers, and brightness temperature profiles for ...
Zallio Luigi   +15 more
doaj   +1 more source

Circumstellar matter in the binary V Puppis

open access: yesThe Astrophysical Journal, 1976
Results are reported for Copernicus observations of the double-lined binary V Puppis in the wavelength region from 1155 to 1310 A with a resolution of 0.2 A. The sharp-lined UV absorption spectrum is found to provide a line of sight dominated by an apparently 'textbook' H II region in a Stromgren sphere surrounding the stars. Several characteristics of
D. G. York, B. Flannery, J. Bahcall
openaire   +1 more source

Vertical Structure of Gas and Dust in Four Debris Disks

open access: yesThe Astrophysical Journal
We present high-spectral-resolution M -band spectra from iSHELL on NASA’s Infrared Telescope Facility along the line of sight to the debris disk host star HD 32297. We also present a Gemini Planet Imager H -band polarimetric image of the HD 131488 debris
Kadin Worthen   +10 more
doaj   +1 more source

Fifteen years of “Sonderforschungsbereich” in Heidelberg: Research on circumstellar matter [PDF]

open access: yesSymposium - International Astronomical Union, 1987
At the end of this year, the Sonderforschungsbereich (Special Collaborative Programme) no. 132 on “Theoretical and Observational Stellar Astronomy” in Heidelberg will terminate after fifteen years. Although 15 years are only 2 1/2 per cent of the age of the University of Heidelberg, which is celebrating its 600 th anniversary this year, they are ...
openaire   +1 more source

Detection of a Molecular Hydrogen Envelope around Nova GK Persei

open access: yesThe Astrophysical Journal Letters
The eruption of Nova Persei 1901 (GK Per) occurred 125 yr ago; remarkably, it still holds major surprises. Using data from the Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer (SPHEREx), we find that it has a ...
D. P. K. Banerjee   +6 more
doaj   +1 more source

The Circumstellar Matter Around OH44.8-2.3

open access: yes, 2000
To appear in ``Asymmetrical Planetary Nebulae II: from Origins to Microstructures,'' ASP Conference Series, Vol. 199, 2000; J.H. Kastner, N. Soker, & S.A.
Bobrowsky, M.   +3 more
openaire   +2 more sources

Circumstellar matter, with particular reference to jets and molecular flows [PDF]

open access: yesSymposium - International Astronomical Union, 1987
Circumstellar matter exists in many forms, such as winds from early and from late type stars, in infra-red sources and OH and H2O masers, in X-ray sources and jets, and molecular flows and Herbig-Haro objects. There is considerable diversity in the nature of the starlike bodies that underlie these phenomena.
openaire   +2 more sources

On the Circumstellar Matter Distribution around Herbig Ae/Be Stars

open access: yesThe Astrophysical Journal, 1997
The spectral energy distributions (SEDs) observed in Herbig Ae/Be stars are critically analyzed in connection with a spherically symmetric model for matter distribution around the central objects. The possibility that the dusty component is described by an MRN-DL mixture (see the work of Mathis, Rumpl, and Nordsiek; Draine and Lee) and is constituted ...
PEZZUTO S.   +2 more
openaire   +2 more sources

Infall Explains the Disk Kinematics of AB Aur without Gravitational Instability

open access: yesThe Astrophysical Journal Letters
Late-stage infall onto protoplanetary disks can produce large-scale spiral arms. In this Letter, we used 3D smoothed particle hydrodynamics and radiative transfer simulations to study the kinematic perturbations induced in disks by infalling material. We
Josh Calcino   +2 more
doaj   +1 more source

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