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Related papers: Molecular hydrogen in the disk of the Herbig Ae st…

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We present high resolution spectroscopic mid-infrared observations of the circumstellar disk around the Herbig Ae star HD97048 with the VLT Imager and Spectrometer for the mid-InfraRed (VISIR). We detect the S(1) pure rotational line of…

Astrophysics · Physics 2009-11-13 C. Martin-Zaidi , P-. O. Lagage , E. Pantin , E. Habart

Mid-IR emission lines of H2 are useful probes to determine the mass of warm gas present in the surface layers of disks. Numerous observations of Herbig Ae/Be stars (HAeBes) have been performed, but only 2 detections of mid-IR H2 toward…

Solar and Stellar Astrophysics · Physics 2015-05-18 C. Martin-Zaidi , J-. C. Augereau , F. Menard , J. Olofsson , A. Carmona , C. Pinte , E. Habart

We observed the Herbig Ae/Be stars UX Ori, HD 34282, HD 100453, HD 101412, HD 104237 and HD 142666, and the T Tauri star HD 319139 and searched for H2 0-0 S(2) emission at 12.278 micron and H2 0-0 S(1) emission at 17.035 micron with VISIR,…

We report on a sensitive search for H2 1-0 S(1), 1-0 S(0) and 2-1 S(1) ro-vibrational emission at 2.12, 2.22 and 2.25 micron in a sample of 15 Herbig Ae/Be stars employing CRIRES, the ESO-VLT near-infrared high-resolution spectrograph, at…

Solar and Stellar Astrophysics · Physics 2015-05-28 A. Carmona , G. van der Plas , M. E. van den Ancker , M. Audard , L. B. F. M Waters , D. Fedele , B. Acke , E. Pantin

Context: Molecular hydrogen (H2) is the most abundant molecule in the circumstellar (CS) environments of young stars, and is a key element in giant planet formation. The measurement of the H2 content provides the most direct probe of the…

Astrophysics · Physics 2009-11-13 C. Martin-Zaidi , E. F. van Dishoeck , J. -C. Augereau , P. -O. Lagage , E. Pantin

The disc around the Herbig Ae/Be star HD 100546 is one of the most extensively studied discs in the southern sky. Although there is a wealth of information about its dust content and composition, not much is known about its gas and large…

Earth and Planetary Astrophysics · Physics 2015-05-18 O. Panić , E. F. van Dishoeck , M. R. Hogerheijde , A. Belloche , R. Güsten , W. Boland , A. Baryshev

We present the results of a coronagraphic scattered-light imaging survey of six young disk candidate stars using the Hubble Space Telescope Advanced Camera for Surveys. The observations made use of the 1.8" occulting spot through the F606W…

We study the sub-AU-scale circumstellar environment of the Herbig Ae star HD144432 with near-infrared (NIR) VLTI/AMBER observations to investigate the structure of its inner dust disk. The interferometric observations were carried out with…

We present observations of far-infrared (50-200 micron) OH and H2O emission of the disk around the Herbig Ae star HD 163296 obtained with Herschel/PACS in the context of the DIGIT key program. In addition to strong [OI] emission, a number…

Solar and Stellar Astrophysics · Physics 2015-06-05 D. Fedele , S. Bruderer , E. F. van Dishoeck , G. J. Herczeg , N. J. Evans , J. Bouwman , Th. Henning , J. Green

We report results from a FUSE survey of interstellar molecular hydrogen (H2) in the Galactic disk toward 139 O-type and early B-type stars at Galactic latitudes $|b| < 10^{\circ}$, with updated photometric and parallax distances. The H2…

Astrophysics of Galaxies · Physics 2021-04-21 J. Michael Shull , Charles W. Danforth , Katherine L. Anderson

We present a determination of the molecular gas mass in the AU Microscopii circumstellar disk. Direct detection of a gas component to the AU Mic disk has proven elusive, with upper limits derived from ultraviolet absorption line and…

Astrophysics · Physics 2009-11-13 Kevin France , Aki Roberge , Roxana E. Lupu , Seth Redfield , Paul D. Feldman

[abridged]CO rovibrational lines are efficient probes of warm molecular gas and can give unique insights into the inner 10 AU of proto-planetary disks. Recent studies have found a relation between the ratio of lines originating from the…

We present ISO-SWS observations of H2 pure-rotational line emission from the disks around low and intermediate mass pre-main-sequence stars as well as from young stars thought to be surrounded by debris disks. We detect `warm' (T ~ 100-200…

Aims: Today, large ground-based instruments, like VISIR on the VLT, providing diffraction-limited (about 0.3 arcsec) images in the mid-infrared where strong PAH features appear enable us to see the flaring structure of the disks around…

Astrophysics · Physics 2007-05-23 Doucet , C. , Habart , E , Pantin , E. , Dullemond , C. , Lagage , P-O , Pinte , C. , Duchêne , G. , Ménard , F.

We report the results of initial FUSE observations of molecular hydrogen (H2) in translucent clouds. These clouds have greater optical depth than any of the diffuse clouds previously observed for far-UV H2 absorption, and provide new…

We present Submillimeter Array observations of the Herbig Ae star HD169142 in 1.3 millimeter continuum emission and 12CO J=2-1 line emission at 1.5 arcsecond resolution that reveal a circumstellar disk. The continuum emission is centered on…

Astrophysics · Physics 2008-11-26 A. Raman , M. Lisanti , D. J. Wilner , C. Qi , M. Hogerheijde

Transitional disks show a lack of excess emission at infrared wavelengths due to a large dust cavity, that is often corroborated by spatially resolved observations at ~ mm wavelengths. We present the first spatially resolved ~ mm-wavelength…

Earth and Planetary Astrophysics · Physics 2016-11-11 Catherine Walsh , Attila Juhász , Gwendolyn Meeus , William R. F. Dent , Luke Maud , Yuri Aikawa , Tom J. Millar , Hideko Nomura

We investigate the physical properties of the inner gaseous disks of the three, hot, Herbig B2e stars, HD 76534, HD 114981 and HD 216629, by modelling CFHT-ESPaDOns spectra using non-LTE radiative transfer codes. We assume that the emission…

Solar and Stellar Astrophysics · Physics 2017-03-08 P. Patel , T. A. A. Sigut , J. D. Landstreet

We have observed warm molecular hydrogen in two nearby edge-on disk galaxies, NGC 4565 and NGC 5907, using the Spitzer high-resolution infrared spectrograph. The 0-0 S(0) 28.2 micron and 0-0 S(1) 17.0 micron pure rotational lines were…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Seppo Laine , Philip N. Appleton , Stephen T. Gottesman , Matthew L. N. Ashby , Catherine A. Garland

We observed molecular hydrogen around a sample of pre-main sequence stars in order to better characterize their gaseous CS environments. We analyzed the FUSE (Far Ultraviolet Spectroscopic Explorer) spectra of a sample of Herbig Ae/Be stars…

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