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CHANG-ES XXXI—A Decade of CHANG-ES: What We Have Learned from Radio Observations of Edge-on Galaxies
DOI: 10.3390/galaxies12030022 Bibcode: 2024Galax..12...22I

Murphy, Eric; Beck, Rainer; Walterbos, Rene +21 more

CHANG-ES (Continuum Halos in Nearby Galaxies—an EVLA Survey) is an ambitious project to target 35 nearby disk galaxies that are edge-on to the line of sight. The orientation permits both the disk and halo regions to be studied. The observations were initially at 1.5 GHz (L-band) and 6.0 GHz (C-band) in a variety of VLA array configurations, and in…

2024 Galaxies
XMM-Newton 10
The Scavenger Hunt for Quasar Samples to Be Used as Cosmological Tools
DOI: 10.3390/galaxies12010004 Bibcode: 2024Galax..12....4D

Bargiacchi, Giada; Dainotti, Maria Giovanna; Lenart, Aleksander Łukasz +1 more

Although the Λ Cold Dark Matter model is the most accredited cosmological model, information at high redshifts (z) between type Ia supernovae (z=2.26) and the Cosmic Microwave Background (z=1100) is crucial to validate this model further. To this end, we have discovered a sample of 1132 quasars up to z=7.54 exhibiting a reduced intrinsic dispersio…

2024 Galaxies
XMM-Newton 10
Planetary Nebula Morphologies Indicate a Jet-Driven Explosion of SN 1987A and Other Core-Collapse Supernovae
DOI: 10.3390/galaxies12030029 Bibcode: 2024Galax..12...29S

Soker, Noam

I demonstrate the usage of planetary nebulae (PNe) to infer that a pair of jets shaped the ejecta of the core-collapse supernova (CCSN) SN 1987A. The main structure of the SN 1987A inner ejecta, the 'keyhole', comprises two low-intensity zones. The northern one has a bright rim on its front, while the southern one has an elongated nozzle. An earli…

2024 Galaxies
eHST JWST 8
Galaxy Groups as the Ultimate Probe of AGN Feedback
DOI: 10.3390/galaxies12030024 Bibcode: 2024Galax..12...24E

Finoguenov, Alexis; Gastaldello, Fabio; O'Sullivan, Ewan +3 more

The co-evolution between supermassive black holes and their environment is most directly traced by the hot atmospheres of dark matter halos. The cooling of the hot atmosphere supplies the central regions with fresh gas, igniting active galactic nuclei (AGN) with long duty cycles. The outflows from the central engine tightly couple with the surroun…

2024 Galaxies
XMM-Newton 6
M 1-92: The Death of an AGB Star Told by Its Isotopic Ratios
DOI: 10.3390/galaxies12050063 Bibcode: 2024Galax..12...63M

Sánchez Contreras, Carmen; Masa, Elisa; Alcolea, Javier +3 more

Ongoing improvements in the sensitivity of sub-mm- and mm-range interferometers and single-dish radio telescopes allow for the increasingly detailed study of AGB and post-AGB objects in molecular species other than CO12

2024 Galaxies
Herschel 2
Correlations between IR Luminosity, Star Formation Rate, and CO Luminosity in the Local Universe
DOI: 10.3390/galaxies12040037 Bibcode: 2024Galax..12...37B

De Zotti, Gianfranco; Bianchi, Simone; Casasola, Viviana +5 more

We exploit the DustPedia sample of galaxies within approximately 40 Mpc, selecting 388 sources, to investigate the correlations between IR luminosity (LIR), the star formation rate (SFR), and the CO(1-0) luminosity (LCO) down to much lower luminosities than reached by previous analyses. We find a sub-linear dependence of the …

2024 Galaxies
Herschel 1
A Dust-Scattering Model for M1-92: A Revised Estimate of the Mass Distribution and Inclination
DOI: 10.3390/galaxies12040044 Bibcode: 2024Galax..12...44L

Morris, Mark R.; Sahai, Raghvendra; Li, Yun Qi

Preplanetary nebulae (PPNe) are formed from mass-ejecting late-stage AGB stars. Much of the light from the star gets scattered or absorbed by dust particles, giving rise to the observed reflection nebula seen at visible and near-IR wavelengths. Precursors to planetary nebulae (PNe), PPNe generally have not yet undergone any ionization by UV radiat…

2024 Galaxies
eHST 1
Fifty Years After the Discovery of the First Stellar-Mass Black Hole: A Review of Cyg X-1
DOI: 10.3390/galaxies12060080 Bibcode: 2024Galax..12...80J

Jiang, Jiachen

Around 50 years ago, the famous bet between Stephen Hawking and Kip Thorne on whether Cyg X-1 hosts a stellar-mass black hole became a well-known story in the history of black hole science. Today, Cyg X-1 is widely recognised as hosting a stellar-mass black hole with a mass of approximately 20 solar masses. With the advancement of X-ray telescopes…

2024 Galaxies
INTEGRAL 0
Steps toward Unraveling the Structure and Formation of Five Polar Ring Galaxies
DOI: 10.3390/galaxies12040042 Bibcode: 2024Galax..12...42L

Kulkarni, Varsha P.; Aller, Monique C.; Lackey, Kyle E.

Polar ring galaxies (PRGs) are unusual relative to common galaxies in that they consist of a central host galaxy—usually a gas-poor, early-type S0 or elliptical galaxy—surrounded by a ring of gas, dust and stars that orbit perpendicular to the major axis of the host. Despite the general quiescence of early-type galaxies (ETGs) and the rings' lack …

2024 Galaxies
eHST 0
A Study of Interstellar Medium in the Line of Sight of Transient Neutron Star Low-Mass X-ray Binary, MXB 1659-298, by Timing and Spectral Analysis
DOI: 10.3390/galaxies12040041 Bibcode: 2024Galax..12...41M

Mahato, Rabindra; Baruah, Monmoyuri; Bhattacharya, Parag

This work is dedicated to the study of interstellar medium (ISM) along the line of sight (LOS) of the transient low-mass X-ray binary, MXB 1659-298, capitalizing the high resolving power of XMM-Newton in the soft energy range. We emphasized the analysis of reflection grating spectrometer (RGS) data in the energy range 0.5–2.15 keV, suitable for th…

2024 Galaxies
XMM-Newton 0