Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
europepmc +1 more source
f(Q) gravity as a possible resolution of the H<sub>0</sub> and S<sub>8</sub> tensions with DESI DR2. [PDF]
Kavya NS, Swagat Mishra S, Sahoo PK.
europepmc +1 more source
Revisiting the Surface Brightness Profile of the Stellar Disk with the Statistical Mechanics of the Self-Gravitating System with the Central Body. [PDF]
Kang DB.
europepmc +1 more source
Primordial black holes and their gravitational-wave signatures. [PDF]
Bagui E +20 more
europepmc +1 more source
Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe
Pérez-González P +21 more
europepmc +1 more source
Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback
Eckert D +21 more
europepmc +1 more source
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Stellar content of the metal-poor galaxy DDO 68
Astronomy Letters, 2014Based on archival Hubble Space Telescope ACS/WFC images, we have performed stellar photometry for the metal-poor galaxy DDO 68. The apparent distributions of stars of different ages and stellarmetallicity determinations indicate that DDO68 is a systemof two galaxies that have different stellar metallicities (Z = 0.004 and 0.001) and are in the stage of
N A Tikhonov +2 more
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We present a first measurement of the stellar mass component of galaxy clusters selected via the Sunyaev-Zel’dovich (SZ) effect, using 3.6 and 4.5 mu m photometry from the Spitzer Space Telescope.
Matt Hilton +2 more
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Stellar content of NGC 404 – The nearest S0 Galaxy
We report $V -$band and $I -$band CCD stellar and surface photometry of the galaxy NGC 404 , taken with HST WFPC2 and the 2.5 m Nordic telescope. The colour-magnitude diagram for the stars in this galaxy is typical of that of spheroidal systems (i.e.
N A Tikhonov, A Aparicio
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LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content [PDF]
International audienceWe present a simultaneous analysis of galaxy cluster scaling relations between weak-lensing mass and multiple cluster observables, across a wide range of wavelengths, that probe both gas and stellar content.
Arya Farahi, A E Evrard, G P Smith
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