Results 181 to 190 of about 16,260 (212)

Characterizing the metabolites of the tyrosine-kinase inhibitor pexidartinib in mouse feces, urine, plasma, and liver. [PDF]

J Pharm Biomed Anal
Qin X, Chen S, Hakenjos JM, Wang J, Guo L, Dogra A, Hu Z, MacKenzie KR, Li F.   +8 more
europepmc   +1 more source

A meta-analysis of complications of thread lifting. [PDF]

Front Surg
Zhou X, Zhuang S.
europepmc   +1 more source

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Neutral Hydrogen near M51

1990
We observed the nearby Sc galaxy M51 (NGC 5194) and its companion NGC 5195 with the VLA in the 21-cm line to study the distribution and kinematics of the HI. M51 is a key object in the study of galaxies: its beautiful spiral structure with the clear separation of the dust lanes and associated radio continuum emission from the bright HII regions and OB ...
A. H. Rots, A. Bosma, J. M. van der Hulst, E. Athanassoula, P. C. Crane   +4 more
openaire   +1 more source

Molecular spiral arms in M51

2008
The controversy surrounding the delineation of molecular spiral structure in the Galaxy emphasizes that spiral structure can best be understood by observing external galaxies with high angular resolution. M51, the galaxy in which spiral structure was first discerned, is the obvious galaxy to observe. Lo et al.
Vogel, S. N., Kulkarni, S. R., Scoville, N. Z., Hester, J.   +3 more
openaire   +2 more sources

Dynamical Status of M51

1990
M51 enjoys a special place in the history of observational astronomy. It was the first galaxy observed to have spiral structure, by Lord Rosse in 1845 using the 72-inch reflector at Burr Castle. Over a century later, M51 became the first galaxy outside the Local Group to be mapped extensively at radio wavelengths by Mathewson, van der Kruit, and Brouw [
openaire   +1 more source

Possibile pianeta extragalattico in M51

2021
È grande come Saturno. Orbita ogni 70 anni attorno a una binaria X a 28 milioni di anni luce da noi, nella Galassia Vortice. Gli indizi della sua esistenza arrivano dalle misure compiute con i telescopi spaziali Chandra e Xmm-Newton per raggi X, e se confermato sarebbe il primo pianeta mai scoperto al di fuori della nostra ...
openaire   +1 more source

Distribution of Molecular Clouds in M51

Publications of the Astronomical Society of Japan, 1985
Abstract Distributions of molecular clouds are calculated in M51 on the assumption that molecular clouds are formed behind the galactic shocks in the spiral arm with postshock velocity, and then move freely along ballistic orbits in the gravitational field of the galaxy modified by the density wave.
Toshiya Kimura, Makoto Tosa
openaire   +1 more source

Molecular Spiral Structure in M51

1990
We present a mosaic map of M51 in the 12CO 1→0 line made with the Owens Valley mm-interferometer. The molecular arms we see are narrow and show an offset relative to the Ha emission. They also show coincidence with the dust lanes. Several interarm emission regions have also been detected, but with very little accompanying Ha emission.
Rand, R. J., Kulkarni, S. R.
openaire   +2 more sources

The transient ultraluminous X-ray source, ULX-4, in M51

Monthly Notices of the Royal Astronomical Society, 2022
Sinan Allak, A Akyuz, Inci Akkaya Oralhan   +2 more
exaly  

M51 ULX-7: superorbital periodicity and constraints on the neutron star magnetic field

Monthly Notices of the Royal Astronomical Society, 2020
G Vasilopoulos
exaly