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相关论文: Circumstellar features in hot DA white dwarfs

200 篇论文

We present the results of a near-IR spectroscopic survey of 110 Class I protostars observed from 0.80 microns to 2.43 microns at a spectroscopic resolution of R=1200. We find that Class I objects exhibit a wide range of lines and the…

星系天体物理 · 物理学 2015-05-19 Michael S. Connelley , Thomas P. Greene

We present imaging and spectroscopic observations with HST (WFPC2, ACS/HRC and STIS), VLT (FORS2) and Keck (HIRES) of the dM8 ultra-cool dwarf DENIS-P J185950.9-370632, located in the R-CrA region. The presence of lithium absorption at…

天体物理学 · 物理学 2010-10-28 H. Bouy , W. Brandner , E. L. Martin , X. Delfosse , F. Allard , I. Baraffe , T. Forveille , R. Demarco

Taking advantage of the now available Gaia EDR3 parallaxes, we carry out an archival {\it Hubble Space Telescope} (HST) far ultraviolet spectroscopic analysis of 10 cataclysmic variable systems, including 5 carefully selected eclipsing…

太阳与恒星天体物理 · 物理学 2022-03-30 Patrick Godon , Edward M. Sion

Results are presented from the first detailed spectroscopic observations of the recently identified intermediate polar RXJ0028.8+5917/V709 Cas. The study of the emission line radial velocities allows us to remove the uncertainties on the…

天体物理学 · 物理学 2009-11-06 J. M. Bonnet-Bidaud , M. Mouchet , D. de Martino , G. Matt , C. Motch

We present a spectro-photometric analysis of 2880 cool white dwarfs within 100 pc of the Sun and cooler than Teff = 10,000 K, with grizy Pan-STARRS photometry and Gaia trigonometric parallaxes available. We also supplement our data sets…

太阳与恒星天体物理 · 物理学 2022-12-28 Alexandre Caron , Pierre Bergeron , Simon Blouin , Sandy K. Leggett

A detailed analysis of the very cool white dwarfs SDSS 1337+00 and LHS 3250 is presented. Model atmosphere calculations with improved collision-induced absorptions by molecular hydrogen indicate that a pure hydrogen composition can be ruled…

天体物理学 · 物理学 2008-11-26 P. Bergeron , S. K. Leggett

We present a spectroscopic survey of 230 white dwarf candidates within 40 pc of the Sun from the William Herschel Telescope and Gran Telescopio Canarias. All candidates were selected from $\textit{Gaia}$ Data Release 2 (DR2) and in almost…

WD J204713.76-125908.9 is a new addition to the small class of white dwarfs with helium-dominated photospheres that exhibit strong Balmer absorption lines and atmospheric metal pollution. The exceptional abundances of hydrogen observed in…

Aiming to perform a study of the warm dust and gas in the luminous blue variable star G79.29+0.46 and its associated nebula, we present infrared Spitzer imaging and spectroscopy, and new CO J=2-->1 and 4-->3 maps obtained with the IRAM 30m…

太阳与恒星天体物理 · 物理学 2015-03-13 F. M. Jiménez-Esteban , J. R. Rizzo , Aina Palau

This letter reports the first JWST spectroscopy of a white dwarf debris disk, giving a preliminary assessment of the salient features, and recommendations for future observations. The polluted and dusty star WD 0145+234 experienced a major…

地球与行星天体物理 · 物理学 2023-12-21 Andrew Swan , Jay Farihi , Kate Y. L. Su , Steven J. Desch

In the line-of-sight toward the DO-type white dwarf RX J0503.9-2854, the density of the interstellar medium (ISM) is very low, and thus the contamination of the stellar spectrum almost negligible. This allows us to identify many metal lines…

太阳与恒星天体物理 · 物理学 2017-02-15 D. Hoyer , T. Rauch , K. Werner , J. W. Kruk , P. Quinet

Among its great findings, the IRAS mission showed the existence of an unidentified mid-IR feature around 21 um. Since its discovery, this feature has been detected in all C-rich proto-PNe of intermediate spectral type (A-G) and - weakly -…

太阳与恒星天体物理 · 物理学 2016-08-03 L. Cerrigone , J. L. Hora , G. Umana , C. Trigilio , A. Hart , G. Fazio

We present the first mid-infrared spectra of two cool white dwarfs obtained with the Spitzer Space Telescope. We also present 3.5-8 micron photometry for 19 cool white dwarfs with 5000K < Teff < 9000K. We perform a detailed model atmosphere…

天体物理学 · 物理学 2009-11-13 Mukremin Kilic , Piotr M. Kowalski , Fergal Mullally , William T. Reach , Ted von Hippel

We perform ground based photometric observations of 22 DA white dwarf stars, 10 already known ZZ Cetis and 12 candidates with atmospheric parameters inside the classical instability strip. We report on the discovery of four new variable DA…

太阳与恒星天体物理 · 物理学 2019-09-25 Alejandra D. Romero , L. Antunes Amaral , T. Klippel , D. Sanmartim , L Fraga , G. Ourique , I. Pelisoli , G. R. Lauffer , S. O. Kepler , D. Koester

We present an analysis of all single white dwarf stars known to exhibit spectroscopic signatures of neutral helium line splitting due to the presence of a strong magnetic field. Using state-of-the-art models taking into account the effects…

太阳与恒星天体物理 · 物理学 2023-02-01 François Hardy , Patrick Dufour , Stefan Jordan

The hierarchical triple system PSR J0337+1715 offers an unprecedented laboratory to study secular evolution of interacting systems and to explore the complicated mass-transfer history that forms millisecond pulsars and helium-core white…

Recent Kepler photometry has revealed that about half of white dwarfs (WDs) have periodic, low-level (~ 1e-4 - 1e-3), optical variations. Hubble Space Telescope (HST) ultraviolet spectroscopy has shown that up to about one half of WDs are…

We present 6300--10100 {\AA} spectra for a sample of 13 T dwarfs observed using LRIS mounted on the Keck I 10m Telescope. A variety of features are identified and analyzed, including pressure-broadened K I and Na I doublets; narrow Cs I and…

天体物理学 · 物理学 2016-08-30 Adam J. Burgasser , J. Davy Kirkpatrick , James Liebert , Adam Burrows

We present a homogeneous analysis of 1023 DBZ/DZ(A) and 319 DQ white dwarf stars taken from the Montreal White Dwarf Database. This represents a significant increase over the previous comprehensive studies on these types of objects. We use…

太阳与恒星天体物理 · 物理学 2020-01-08 S. Coutu , P. Dufour , P. Bergeron , S. Blouin , E. Loranger , N. F. Allard , B. H Dunlap

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…

天体物理学 · 物理学 2009-10-31 Rafael Millan-Gabet , F. Peter Schloerb , Wesley A. Traub