Results 91 to 100 of about 553,808 (287)

The Millennium Galaxy Catalogue: the local supermassive black hole mass function in early- and late-type galaxies [PDF]

open access: yes, 2007
We provide a new estimate of the local supermassive black hole mass function using (i) the empirical relation between supermassive black hole mass and the Sersic index of the host spheroidal stellar system and (ii) the measured (spheroid) Sersic indices ...
A. Graham, S. Driver, P. Allen, J. Liske
semanticscholar   +1 more source

The Geography of Success: A Spatial Analysis of Export Intensity in the Italian Wine Industry

open access: yesAgribusiness, EarlyView.
ABSTRACT This paper investigates the paradox of how Italy's fragmented, SME‐dominated wine industry achieves global export success. Moving beyond purely firm‐centric explanations, we test whether export intensity is spatially dependent, clustering geographically in regional ecosystems.
Nicolas Depetris Chauvin, Jonas Di Vita
wiley   +1 more source

Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View

open access: yesThe Astrophysical Journal, 2023
We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST.
Luca Costantin   +18 more
doaj   +1 more source

Stellar Populations in the Nuclei of Late‐Type Spiral Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2006
ApJ submitted (original submission Oct 19, 2005, present version includes changes based on referee recommendations).
Walcher, C. J.   +7 more
openaire   +4 more sources

The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5

open access: yes, 2005
We measure the evolution of clustering for galaxies with different spectral types from 6495 galaxies with 17 ...
Adami, C.   +49 more
core   +2 more sources

Tracing the Mass-Dependent Star Formation History of Late-Type Galaxies Using X-Ray Emission: Results from the Chandra Deep Fields [PDF]

open access: yes, 2008
We report on the X-ray evolution over the last ≈9 Gyr of cosmic history (i.e., since z = 1.4) of late-type galaxy populations in the Chandra Deep Field-North and Extended Chandra Deep Field-South (CDF-N and E-CDF-S, respectively; jointly CDFs) survey ...
B. Lehmer   +14 more
semanticscholar   +1 more source

Repeating Nuclear Transients From Repeating Partial Tidal Disruption Events

open access: yesAstronomische Nachrichten, EarlyView.
ABSTRACT Extragalactic nuclear transients that exhibit repeating outbursts can be modeled as the repeated dynamical interaction between bound stars and supermassive black holes (SMBHs). A subset of these transients, with recurrence timescales of months‐to‐years, have been explained as accretion flares from the repeated tidal stripping of a star by an ...
Ananya Bandopadhyay   +4 more
wiley   +1 more source

AMUSE-Antlia. I. Nuclear X-Ray Properties of Early-type Galaxies in a Dynamically Young Galaxy Cluster

open access: yesThe Astrophysical Journal, 2023
To understand the formation and growth of supermassive black holes (SMBHs) and their coevolution with host galaxies, it is essential to know the impact of environment on the activity of active galactic nuclei (AGNs).
Zhensong Hu   +16 more
doaj   +1 more source

[CII] at 158 mu m as a star formation tracer in late-type galaxies [PDF]

open access: yes, 2002
We present a calibration of the massive star formation rate vs. [CII] luminosity relation based on a sample of nearby, late-type galaxies observed with ISO-LWS and imaged in the Halpha+[NII] line. The relation holds for far-IR luminosities 10^8 < L_{FIR}
A. Boselli   +3 more
semanticscholar   +1 more source

Quantifying the Impact of Relativistic Precession on Tidal Disruption Event Light Curves

open access: yesAstronomische Nachrichten, EarlyView.
ABSTRACT The tidal field of a black hole can turn a star into a gas stream whose orbit can precess, especially if the a black hole is rapidly spinning. In this work, we investigate the impact of precession on the light curves of tidal disruption events (TDE).
Diego Calderón   +4 more
wiley   +1 more source

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