Results 91 to 100 of about 12,515 (261)
Chemistry in Externally FUV-irradiated Disks in the Outskirts of the Orion Nebula Cluster
Most stars are born in stellar clusters, and their protoplanetary disks, which are the birthplaces of planets, can, therefore, be affected by the radiation of nearby massive stars.
Javiera K. Díaz-Berríos +6 more
doaj +1 more source
The Orion Nebula in the mid-IR
34 pages, 22 figures, 5 tables, AJ in ...
ROBBERTO M. +8 more
openaire +3 more sources
The Orion Nebula Cluster (ONC) is the closest site of very young (∼1 Myr) massive star formation The ONC hosts more than 1600 young and X-ray bright stars with masses ranging from ∼0.1–35 M _⊙ .
Norbert S. Schulz +12 more
doaj +1 more source
Relationship between CH3OD Abundance and Temperature in the Orion KL Nebula. [PDF]
Wilkins OH, Blake GA.
europepmc +1 more source
A Census of the Carina Nebula -- II. Energy Budget and Global Properties of the Nebulosity
The first paper in this series took a direct census of energy input from the known OB stars in the Carina Nebula, and in this paper we study the global properties of the surrounding nebulosity.
Hester, K. J. Brooks, N. Smith
core +1 more source
MILAN Sky Survey, a dataset of raw deep sky images captured during one year with a Stellina automated telescope. [PDF]
Parisot O +5 more
europepmc +1 more source
Stellar Proper Motions in the Orion Nebula Cluster [PDF]
Dongwon Kim +7 more
openalex +1 more source
A Radio Counterpart to a Jupiter-mass Binary Object in Orion
Using James Webb Space Telescope near-infrared data of the inner Orion Nebula, Pearson & McCaughrean detected 40 Jupiter-mass binary objects (JuMBOs).
Luis F. Rodríguez +2 more
doaj +1 more source
Editorial: Automated data curation and data governance automation. [PDF]
Talburt JR, Ehrlinger L, Magruder J.
europepmc +1 more source
A Keck High-Resolution Spectroscopic Study of the Orion Nebula Proplyds [PDF]
W. J. Henney, C. R. O’dell
openalex +1 more source

