Results 1 to 10 of about 3,080,831 (379)

Witnessing the emergence of a carbon star [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2015
Abstract During the late stages of their evolution, Sun-like stars bring the products of nuclear burning to the surface. Most of the carbon in the Universe is believed to originate from stars with masses up to a few solar masses. Although there is a chemical dichotomy between oxygen-rich and carbon-rich evolved stars, the dredge-up ...
David Jones   +13 more
openaire   +8 more sources

Evolution of Neutron-Star, Carbon-Oxygen White-Dwarf Binaries [PDF]

open access: bronze, 2000
At least one, but more likely two or more, eccentric neutron-star, carbon-oxygen white-dwarf binaries with an unrecycled pulsar have been observed.
Braun H.   +20 more
core   +4 more sources

Prefabricated building construction in materialization phase as catalysts for hotel low-carbon transitions via hybrid computational visualization algorithms [PDF]

open access: yesScientific Reports
This study examines the carbon emissions of star-rated hotels in Hangzhou, comparing the environmental impact of prefabricated construction (PC) and conventional construction (CC) methodologies.
Gangwei Cai, Xiaoting Guo, Yuguang Sun
doaj   +2 more sources

Carbon star survey in the Local Group. VII. NGC 3109 a galaxy without a stellar halo [PDF]

open access: bronze, 2003
We present a CFH12K wide field survey of the carbon star population in and around NGC 3109. Carbon stars, the brightest members of the intermediate-age population, were found nearly exclusively in and near the disk of NGC 3109, ruling out the existence ...
Albert   +29 more
core   +2 more sources

High-Resolution Spectroscopy of Cool Carbon-Rich and Metal-Poor Star HD 209621 [PDF]

open access: hybridOpen Astronomy, 2012
Element abundances for HD 209621 obtained earlier display significant discrepancies, especially in the case of CNO and neutron-capture elements. Therefore we performed a detailed analysis of chemical composition of this star using a new high-resolution ...
Matrozis E., Začs L., Barzdis A.
doaj   +2 more sources

Carbon emission reduction calculation for the green transformation of traditional hotel design

open access: yesFrontiers in Energy Research, 2022
The green transformation design of traditional hotels aims to reduce the consumption of materials and energy and reduce the emission of harmful substances.
Jing Qiu   +4 more
doaj   +1 more source

TU Tau B: The Peculiar “Eclipse” of a Possible Proto-barium Giant

open access: yesThe Astronomical Journal, 2023
TU Tau (=HD 38218 = HIP 27135) is a binary system consisting of a C-N carbon star primary and an A-type secondary. We report on new photometry and spectroscopy which tracked the recent disappearance of the A-star secondary.
Richard O. Gray   +28 more
doaj   +1 more source

The Carbon Stars Adventure [PDF]

open access: yesProceedings of the International Astronomical Union, 2015
AbstractWe compare in a systematic way spectrometric, photometric and mid-infrared (VLTI/MIDI) interferometric measurements with different types of model atmospheres. Self-consistent dynamic model atmospheres in particular were used to interpret in a consistent way the dynamic behavior of gas and dust.
Rau, Gioia   +6 more
openaire   +3 more sources

On the formation of carbon stars [PDF]

open access: yesThe Astrophysical Journal, 1990
The effect of the mass loss on the formation of carbon stars is investigated using different mass-loss formulas including one proposed in this paper, and the results of different formulas are compared with the observed properties of C stars. It is shown that the new formula reproduces well the observed luminosity distribution of AGB stars, the initial ...
Bryan, GL, Volk, K, Kwok, S
openaire   +4 more sources

The Puzzling Properties of the MACS1149-JD1 Galaxy at z = 9.11

open access: yesThe Astrophysical Journal Letters, 2023
We analyze new JWST NIRCam and NIRSpec data on the redshift 9.11 galaxy MACS1149-JD1 (hereafter JD1). Our NIRCam imaging data reveal that JD1 comprises three spatially distinct components. Our spectroscopic data indicate that JD1 appears dust free but is
Massimo Stiavelli   +8 more
doaj   +1 more source

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