Results 101 to 110 of about 1,583 (233)

Modeling Ionized Gas in the Small Magellanic Cloud: The Wolf–Rayet Nebula N76

The Astrophysical Journal
We present Cloudy modeling of infrared emission lines in the Wolf–Rayet (WR) nebula N76 caused by one of the most luminous and hottest WR stars in the low metallicity Small Magellanic Cloud.
Elizabeth Tarantino, Alberto D. Bolatto, Rémy Indebetouw, Mónica Rubio, Karin M. Sandstrom, J.-D T. Smith, Daniel Stapleton, Mark Wolfire   +7 more
doaj   +1 more source

Complex organosulfur molecules on comet 67P: Evidence from the ROSINA measurements and insights from laboratory simulations. [PDF]

Sci Adv, 2023
Mahjoub A, Altwegg K, Poston MJ, Rubin M, Hodyss R, Choukroun M, Ehlmann BL, Hänni N, Brown ME, Blacksberg J, Eiler JM, Hand KP.   +11 more
europepmc   +1 more source

Extended X‐Ray Emission from the Planetary Nebula BD +30o3639 [PDF]

, 2000
D. A. Leahy, Sun Kwok, D. Yin
openalex   +1 more source

Laboratory IR Spectra of the Ionic Oxidized Fullerenes C₆₀O⁺ and C₆₀OH. [PDF]

J Phys Chem A, 2022
Palotás J, Martens J, Berden G, Oomens J.   +3 more
europepmc   +1 more source

Likely Detection of GeV γ-Ray Emission from Pulsar Wind Nebula G32.64+0.53 with Fermi-LAT

The Astrophysical Journal
In this study, we report the likely GeV γ -ray emissions originating from the pulsar PSR J1849-0001's pulsar wind nebula (PWN) G32.64+0.53. Our analysis covers approximately 14.7 yr of data from the Fermi Large Area Telescope Pass 8.
Yifan Xiao, Keyao Wu, Jun Fang
doaj   +1 more source

Detection of molecular hydrogen quadrupole emission in the Orion Nebula

, 1976
III Gautier T. N., U. Fink, H. P. Larson, R. R. Treffers   +3 more
openalex   +1 more source

Chondrule-like objects and Ca-Al-rich inclusions in Ryugu may potentially be the oldest Solar System materials. [PDF]

Nat Commun, 2023
Nakashima D, Nakamura T, Zhang M, Kita NT, Mikouchi T, Yoshida H, Enokido Y, Morita T, Kikuiri M, Amano K, Kagawa E, Yada T, Nishimura M, Nakato A, Miyazaki A, Yogata K, Abe M, Okada T, Usui T, Yoshikawa M, Saiki T, Tanaka S, Nakazawa S, Terui F, Yurimoto H, Noguchi T, Yabuta H, Naraoka H, Okazaki R, Sakamoto K, Watanabe SI, Tachibana S, Tsuda Y.   +32 more
europepmc   +1 more source

On the molecular hydrogen emission at the Orion Nebula

, 1977
John Kwan
openalex   +1 more source

Measurement and Interpretation of Deuterium‐Line Emission in the Orion Nebula [PDF]

, 2001
C. R. O’dell, G. J. Ferland, W. J. Henney   +2 more
openalex   +1 more source

FAST Search for Circumstellar Atomic Hydrogen. III. Planetary Nebulae at Galactic Latitudes ∣b∣ ≥ 10°

The Astronomical Journal
The detection of circumstellar atomic hydrogen (H i ) via the 21 cm line remains a persistent challenge in planetary nebula (PN) studies, primarily due to contamination from ubiquitous interstellar H i 21 cm emission. In this paper, we report the results
Xu-Jia Ouyang, Yong Zhang, Albert Zijlstra, Chuan-Peng Zhang, Jun-ichi Nakashima, Quentin A. Parker, Xiao-Hu Li   +6 more
doaj   +1 more source