Results 131 to 140 of about 56,155 (210)

Exploring the universe through dusty visions. [PDF]

Philos Trans A Math Phys Eng Sci
Khawaja N, Klenner F, Szalay J, Kobayashi M, Briois C, Mann I.   +5 more
europepmc   +1 more source

Anomalous Extinction and Diffuse Interstellar Bands In the Direction of 2 Be Stars

, 1992
The Be stars HD 44458 and HD 63462, characterized by peculiar extinction curves, were observed spectroscopically in the range of well-known diffuse interstellar bands - DIBs - (5780, 5797, 6196 and 6203 angstrom). The lack of some of the diffuse features
J. KRELOWSKI, I. PORCEDDU, BENVENUTI, PIERO   +2 more
core  

Observations of Exocomets. [PDF]

Space Sci Rev
Korth J, Norazman A, Bendahan-West R, Kennedy G, Madurga Favieres C, Iglesias D, Shubina O, Xu S, Roth NX.   +8 more
europepmc   +1 more source

A binary-related origin mediated by environmental conditions for blue straggler stars. [PDF]

Nat Commun
Ferraro FR, Lanzoni B, Vesperini E, Dalessandro E, Cadelano M, Pallanca C, Beccari G, Nardiello D, Libralato M, Piotto G.   +9 more
europepmc   +1 more source

New Electronic Transition of Ovalene in Solid <i>para</i>-H₂: The S₁-S₀ Transition with Its Origin at 19 400 cm^-1. [PDF]

J Phys Chem Lett
Weber I, Langner J, Witek HA, Lee YP.
europepmc   +1 more source

Variations in the Law of Interstellar Reddening.

The Astronomical Journal, 1963
openaire   +2 more sources

DIFFUSE INTERSTELLAR BAND AT 8620 angstrom IN RAVE: A NEW METHOD FOR DETECTING THE DIFFUSE INTERSTELLAR BAND IN SPECTRA OF COOL STAR

, 2013
Diffuse interstellar bands (DIBs) 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 their distribution
Bienayme, O, Gilmore, G, Zwitter, T, Seabroke, G, Kos, J, Bland-Hawthorn, J, Binney, J, Gibson, BK, Kordopatis, G, Parker, Q, Steinmetz, M, Reid, WA, Siebert, A, Grebel, EK, Watson, F, Freeman, KC, Siviero, A, Wyse, RFG, Navarro, JF   +18 more
core  

Precision analysis of NGC 2158 with Gaia DR3. [PDF]

Sci Rep
Ahmed NM, Tadross AL.
europepmc   +1 more source

The abundances of carbon and nitrogen in the atmospheres of classical Be stars. [PDF]

Astrophys Space Sci
Peters GJ, Gayley KG, Rast RG, Vink JS, Drake JJ.   +4 more
europepmc   +1 more source

Machine learning-enabled membership determination of open cluster AH03_J0748-26.9 using Gaia DR3 astrometry. [PDF]

Sci Rep
Badawy WA, Abdel Rahman HI.
europepmc   +1 more source