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相关论文: A Catalog of Diffuse Interstellar Bands in the Spe…

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This study presents the largest mid-infrared spectral catalog of Herbig Ae/Be stars to date, containing the Spitzer Infrared Spectrograph spectra of 126 stars. Based on the catalog analysis, two prominent infrared vibrational modes of…

太阳与恒星天体物理 · 物理学 2023-05-31 R. Arun , Blesson Mathew , P. Manoj , G. Maheswar , B. Shridharan , Sreeja S. Kartha , Mayank Narang

We present a new high signal to noise ratio spectroscopic survey of the Northern hemisphere to probe the Local Bubble and its surroundings using the $\lambda 5780$ \AA\ and $\lambda 5797$ \AA\ Diffuse Interstellar Bands (DIBs). We observed…

The formation of dust gaps in protoplanetary disks is one of the most important signposts of disk evolution and possibly the formation of planets. We aim to characterize the 'flaring' disk structure around the Herbig Ae/Be stars HD 100453…

太阳与恒星天体物理 · 物理学 2016-04-20 S. Khalafinejad , K. M. Maaskant , N. Marinas , A. G. G. M Tielens

Large fullerenes and fullerene-based molecules have been proposed as carriers of diffuse interstellar bands (DIBs). The recent detection of the most common fullerenes (C60 and C70) around some planetary nebulae (PNe) now enable us to study…

太阳与恒星天体物理 · 物理学 2014-12-24 J. J. Diaz-Luis , D. A. Garcia-Hernandez , N. Kameswara Rao , A. Manchado , F. Cataldo

This study theoretically predicts the specific Polycyclic Aromatic Hydrocarbon (PAH) molecules to reproduce both astronomically observed Infrared Bands (IR) and Diffuse Interstellar Bands (DIB). In our recent paper, we could reproduce IR by…

星系天体物理 · 物理学 2023-11-23 Norio Ota

LB-1 has variously been proposed as either an X-ray dim B-type star plus black hole (B+BH) binary, or a Be star plus an inflated stripped star (Be+Bstr) binary. The Space Telescope Imaging Spectrograph (STIS) on board HST was used to obtain…

New HST/STIS optical spectra were obtained for a sample of early type stars with existing IUE UV spectra. These data were used to construct optical extinction curves whose general properties are discussed elsewhere. In this paper, we…

太阳与恒星天体物理 · 物理学 2020-03-11 D. Massa , E. L. Fitzpatrick , K. D. Gordon

In 2015, Campbell et al. (Nature 523, 322) presented spectroscopic laboratory gas phase data for the fullerene cation, C$_{60}^+$, that coincide with reported astronomical spectra of two diffuse interstellar band (DIB) features at 9633 and…

We present Infrared Space Observatory (ISO) spectra of fourteen isolated Herbig Ae/Be (HAEBE) stars, to study the characteristics of their circumstellar dust. These spectra show large star-to-star differences, in the emission features of…

天体物理学 · 物理学 2014-10-13 G. Meeus , L. B. F. M. Waters , J. Bouwman , M. E. van den Ancker , C. Waelkens , K. Malfait

We search high-resolution and high-quality VLT/UVES optical spectra of the hot R Coronae Borealis (RCB) star DY Cen for electronic transitions of the C60 molecule and diffuse interstellar bands (DIBs). We report the non-detection of the…

太阳与恒星天体物理 · 物理学 2015-06-11 D. A. Garcia-Hernandez , N. Kameswara Rao , David L. Lambert

HD 179821 is an evolved star of unknown progenitor mass range (either post-Asymptotic Giant Branch or post-Red Supergiant) exhibiting a double peaked spectral energy distribution (SED) with a sharp rise from $\sim8-20$ $\mu$m. Such features…

天体物理学 · 物理学 2009-11-13 J. Nordhaus , I. Minchev , B. Sargent , W. Forrest , E. G. Blackman , O. De Marco , J. Kastner , B. Balick , A. Frank

Absorption spectra toward Herschel 36 for the A^1Pi <-- X^1Sigma transitions of CH+ in the J=1 excited rotational level and the A^2Delta <-- X^2Pi transition of CH in the J=3/2 excited fine structure level have been analyzed. These excited…

星系天体物理 · 物理学 2017-08-30 Takeshi Oka , Daniel E. Welty , Sean Johnson , Donald G. York , Julie Dahlstrom , L. M. Hobbs

Ever since their first detection over 100 years ago, the mysterious diffuse interstellar bands (DIBs), a set of several hundred broad absorption features seen against distant stars in the optical and near infrared wavelength range, largely…

星系天体物理 · 物理学 2021-12-22 T. P. Nie , F. Y. Xiang , Aigen Li

High resolution far-ultraviolet spectra of the O-type subdwarf BD +28 4211 were obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE) to measure the interstellar deuterium, nitrogen, and oxygen abundances in this direction. The…

The first gas-phase infrared spectra of two isolated astronomically relevant and large PAH cations - diindenoperylene (DIP) and dicoronylene (DC) - in the 530$-$1800 cm$^{-1}$ (18.9$-$5.6 $\mu$m) range - are presented. Vibrational band…

天体物理仪器与方法 · 物理学 2018-09-25 Junfeng Zhen , Alessandra Candian , Pablo Castellanos , Jordy Bouwman , Harold Linnartz , Alexander G. G. M. Tielens

Using the Mid-Infrared Spectrometer on board the Infrared Telescope in Space and the low-resolution grating spectrometer (PHT-S) on board the Infrared Space Observatory, we obtained 820 mid-infrared (5 to 12 $\mu$m) spectra of the diffuse…

天体物理学 · 物理学 2009-10-31 Kin-Wing Chan , T. L. Roellig , T. Onaka , M. Mizutani , K. Okumura , I. Yamamura , T. Tanabe , H. Shibai , T. Nakagawa , H. Okuda

We present mid IR spectro-photometric imaging of a sample of eight nearby ($D \leq 240$pc) Herbig Ae/Be stars. The spectra are dominated by photospheric emission (HR6000), featureless infrared excess emission (T~Cha), broad silicate…

天体物理学 · 物理学 2007-05-23 R. Siebenmorgen , T. Prusti , A. Natta , Th. Mueller

We have obtained high resolution optical spectroscopy of 10 reddened O-type stars with UVES at VLT to search for interstellar bands of the naphthalene cation (C$_{10}$H$_{8}$$^+$) in the intervening clouds. No absorption features were…

星系天体物理 · 物理学 2015-05-30 Susana Iglesias-Groth , Jonay I. González Hernández , Arturo Manchado

We have used the COBE DIRBE database to derive near- and mid-infrared light curves for a well-defined sample of 38 infrared-bright Mira variable stars, and compared with optical data from the AAVSO. In general, the 3.5 micron and 4.9 micron…

天体物理学 · 物理学 2009-11-07 Beverly J. Smith , D. Leisawitz , M. W. Castelaz , D. Luttermoser

Diffuse Galactic light has been observed in the optical since the 1930s. We propose that, when observed in the optical with deep imaging surveys, it can be used as a tracer of the turbulent cascade in the diffuse interstellar medium (ISM),…

星系天体物理 · 物理学 2016-08-31 M. -A. Miville-Deschenes , P. -A. Duc , F. Marleau , J. -C. Cuillandre , P. Didelon , S. Gwyn , E. Karabal