Results 51 to 60 of about 35,694,720 (305)

JWST Peers into the Class I Protostar TMC1A: Atomic Jet and Spatially Resolved Dissociative Shock Region

open access: yesThe Astrophysical Journal Letters, 2023
Outflows and winds launched from young stars play a crucial role in the evolution of protostars and the early stages of planet formation. However, the specific details of the mechanism behind these phenomena, including how they affect the protoplanetary ...
D. Harsono   +8 more
doaj   +1 more source

21-cm H I emission from the Damped Lyman- [PDF]

open access: yes, 2001
We detect 21-cm emission from the Low Surface Brightness (LSB) galaxy SBS 1543+593, which gives rise to a Damped-Lyα (DLyα) absorption line in the spectrum of the background QSO HS 1543+5921 ($z_{\rm e} = 0.807$).
W. Huchtmeier   +9 more
core   +1 more source

Irregular changes in H α emission line of V423 Aur observed by LAMOST Medium-Resolution Spectrographs [PDF]

open access: yesResearch in Astronomy and Astrophysics, 2020
Abstract We obtained seven spectra of the Be star V423 Aur on 2017 Dec. 5 using the LAMOST Medium-Resolution Spectrograph with exposures from 600 to 1200 seconds. These spectra show the irregular H α emission line profile variations (LPVs). In the seven spectra, from the 4th
Wu, Chao-Jian   +10 more
openaire   +2 more sources

Going viral − Virus‐targeting nanobodies for research, diagnostics and therapy

open access: yesFEBS Letters, EarlyView.
The increasing prevalence of viral diseases represents a major threat for global human health. Nanobodies, small binding fragments derived from camelid heavy‐chain antibodies, offer versatile tools for viral research, diagnostics, and antiviral therapy.
Domenic Ebert, Ulrich Rothbauer
wiley   +1 more source

Two extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey

open access: yes, 2006
We present spectroscopic observations with the 3.6 m ESO telescope of two emission-line galaxies, J2104-0035 and J0113+0052, selected from the Data Release 4 (DR4) of the Sloan Digital Sky Survey (SDSS).
Guseva, N. G.   +9 more
core   +1 more source

Expanded Generalized Needlet Internal Linear Combination (eGNILC) Framework for the 21 cm Foreground Removal

open access: yesThe Astrophysical Journal Supplement Series
The Generalized Needlet Internal Linear Combination (GNILC) method is a nonparametric component separation algorithm to remove the foreground contamination of the 21 cm intensity mapping data.
Wei-Ming Dai, Yin-Zhe Ma
doaj   +1 more source

Detection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment

open access: yesThe Astrophysical Journal, 2023
We present a detection of 21 cm emission from large-scale structure (LSS) between redshift 0.78 and 1.43 made with the Canadian Hydrogen Intensity Mapping Experiment.
The CHIME Collaboration   +32 more
doaj   +1 more source

Inner Warm Disk of ESO Hα 279a Revealed by NA i and CO Overtone Emission Lines [PDF]

open access: yesThe Astrophysical Journal, 2017
Abstract We present an analysis of near-infrared, high-resolution spectroscopy toward the flat-spectrum young stellar object (YSO) ESO Hα 279a (∼1.5M ⊙) in the Serpens star-forming region at a distance of 429 pc. Using the Immersion GRating INfrared Spectrometer (IGRINS; R ≈ 45,000), we detect emission lines originating
A-Ran Lyo   +22 more
openaire   +2 more sources

IMPDH inhibition enhances cytarabine efficacy in SAMHD1‐expressing leukaemia cells via guanine nucleotide depletion

open access: yesMolecular Oncology, EarlyView.
Cytarabine is a key therapy for acute myeloid leukaemia (AML), but its efficacy is limited by the dNTPase SAMHD1, which hydrolyses its active metabolite. Screening nucleotide biosynthesis inhibitors revealed that IMPDH inhibitors selectively sensitise SAMHD1‐proficient AML cells to cytarabine.
Miriam Yagüe‐Capilla   +9 more
wiley   +1 more source

$\text{H}\alpha$ dots: A catalog of faint emission-line objects discovered in narrowband images [PDF]

open access: yes, 2012
During a wide-field narrowband $\text{H}\alpha$ imaging survey, we noted the presence of numerous isolated emission-line point sources in the data. These objects could represent ultra-low-luminosity galaxies at low-redshift (detection via $\text{H}\alpha$
Kellar, J.A.   +4 more
core   +1 more source

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