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We have used spectra of hot stars from the RAVE Survey in order to investigate the visibility and properties of five diffuse interstellar bands previously reported in the literature. The RAVE spectroscopic survey for Galactic structure and…

The gas-phase optical absorption spectrum of a thiophenoxy radical (C6H5S), a diffuse interstellar band (DIB) candidate molecule, was observed in the discharge of thiophenol using a cavity ringdown spectrometer. The ground-state rotational…

Solar and Stellar Astrophysics · Physics 2015-06-22 Mitsunori Araki , Kei Niwayama , Koichi Tsukiyama

Diffuse interstellar bands are usually observed in spectra of hot stars, where interstellar lines are rarely blended with stellar ones. The need for hot stars is a strong limitation in the number of sightlines we can observe and the…

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…

Astrophysics of Galaxies · Physics 2023-11-23 Norio Ota

The sources behind numerous key diffuse interstellar bands (DIBs) remain elusive, and thus evidence is presented here that a family of seven anionic hydrogen atomic clusters (H(-)2n+1, n = 1 to 7) are pertinent contributors. Configuration…

Astrophysics of Galaxies · Physics 2019-12-30 Lulu Huang , Cherif F. Matta , Daniel Majaess , Tina Harriott , Joseph Capitani , Lou Massa

We develop the theory of interstellar scintillation as caused by an irregular plasma having a power-law spatial density spectrum with a spectral exponent of 4 corresponding to a medium with abrupt changes in its density. An ``outer scale''…

Astrophysics · Physics 2009-10-31 Hendrik Lambert , Barney Rickett

Tidal debris from Galactic satellites generally forms one-dimensional elongated streams, since nearby Galactic orbits have almost identical frequency ratios. We show that the situation is different for orbits close to the Galactic disc,…

Astrophysics of Galaxies · Physics 2018-06-29 Walter Dehnen , Hasanuddin

Following the tentative identification of the blue luminescence in the Red Rectangle by Vijh et al. (2005), we compute absolute fluxes for the vibrational IR emission and phosphorescence bands of three small polycyclic aromatic…

Astrophysics · Physics 2009-11-11 G. Mulas , G. Malloci , C. Joblin , D. Toublanc

This paper calls attention to the relevance of Raman scattering by atomic hydrogen to three optical and near/mid-infrared spectral features of HI clouds: extended red emission (ERE), diffuse interstellar bands (DIBs), and the unidentified…

Astrophysics of Galaxies · Physics 2021-08-25 Frederic Zagury

We present the first sample of diffuse interstellar bands (DIBs) in the nearby galaxy M33. Studying DIBs in other galaxies allows the behaviour of the carriers to be examined under interstellar conditions which can be quite different from…

Astrophysics of Galaxies · Physics 2015-06-16 Keith T. Smith , Martin A. Cordiner , Christopher J. Evans , Nick L. J. Cox , Peter J. Sarre

We carried out high-sensitivity spectropolarimetric observations of the central star of the Red Rectangle proto-planetary nebula with the aim of constraining the mechanism that gives its biconical shape. The stellar light of the central…

Solar and Stellar Astrophysics · Physics 2015-06-23 M. J. Martinez Gonzalez , A. Asensio Ramos , R. Manso Sainz , R. L. M. Corradi , F. Leone

The carriers of diffuse interstellar bands are still mysterious species. There exist many arguments that diffuse bands at 5797 and 5850 angstroms have the same carrier. Using high-resolution spectra of few dozens of reddened stars we have…

Astrophysics · Physics 2007-05-23 Katarzyna Bryndal , Bogdan Wszołek

The origin of the narrow optical emission bands seen toward the Red Rectangle is not yet understood. In this paper we investigate further the proposal that these are due to luminescence of large carbonaceous molecules. Polarised signals of…

Astrophysics of Galaxies · Physics 2014-08-11 N. L. J. Cox , B. H. Foing , J. Cami , P. J. Sarre

We use more than 872,000 mid-to-high resolution (R $\sim$ 20,000) spectra of stars from the GALAH survey to discern the spectra of diffuse interstellar bands (DIBs). We use four windows with the wavelength range from 4718 to 4903, 5649 to…

We present spectroscopic VLT/UVES observations of two emerging supernovae, the Type Ia SN 2001el and the Type II SN 2003hn, in the spiral galaxy NGC 1448. Our high resolution and high signal-to-noise spectra display atomic lines of Ca II,…

We identify nearby disk galaxies with optical structural parameters similar to those of intermediate-redshift compact blue galaxies. By comparing HI and optical emission-line widths, we show that the optical widths substantially…

Astrophysics · Physics 2009-11-06 Elizabeth J. Barton , Liese van Zee

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…

We studied the influence of a massive star on a mid-infrared bubble and its surrounding gas in the IRAS\,16489-4431 star-forming region using multi-wavelength data. The {\it Spitzer} mid-infrared band images revealed the shocked nature of…

Astrophysics of Galaxies · Physics 2024-05-29 Ariful Hoque , Tapas Baug , Lokesh Dewangan , Ke Wang , Tie Liu , Soumen Mondal

Stellar spectroscopic surveys may bring useful statistical information on the links between Diffuse Interstellar Bands (DIBs) and interstellar environment. DIB databases can also be used as a complementary tool for locating interstellar…

Astrophysics of Galaxies · Physics 2015-06-15 Lucky Puspitarini , Rosine Lallement , Hui-Chen Chen

Here we report our discovery of a band of blue luminescence (BL) in the Red Rectangle (RR) nebula. This enigmatic proto-planetary nebula is also one of the brightest known sources of extended red emission as well as of unidentified…

Astrophysics · Physics 2009-11-10 Uma P. Vijh , Adolf N. Witt , Karl D. Gordon
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