Search Results - "Meidt, S. E"
-
1
RESOLVING THE FAR-IR LINE DEFICIT: PHOTOELECTRIC HEATING AND FAR-IR LINE COOLING IN NGC 1097 AND NGC 4559
Published in The Astrophysical journal (01-03-2012)“…The physical state of interstellar gas and dust is dependent on the processes which heat and cool this medium. To probe heating and cooling of the interstellar…”
Get full text
Journal Article -
2
Mapping Metallicity Variations across Nearby Galaxy Disks
Published in The Astrophysical journal (10-12-2019)“…The distribution of metals within a galaxy traces the baryon cycle and the buildup of galactic disks, but the detailed gas phase metallicity distribution…”
Get full text
Journal Article -
3
The lifetime of grand design
Published in Monthly notices of the Royal Astronomical Society. Letters (01-02-2006)“…The lifetime of the structure in grand design spiral galaxies is observationally ill-determined, but is essentially set by how accurately the rotation of the…”
Get full text
Journal Article -
4
The spatial relation between young star clusters and molecular clouds in M51 with LEGUS
Published in Monthly notices of the Royal Astronomical Society (11-03-2019)“…We present a study correlating the spatial locations of young star clusters with those of molecular clouds in NGC 5194, in order to investigate the time-scale…”
Get full text
Journal Article -
5
Comparing the pre-SNe feedback and environmental pressures for 6000 H ii regions across 19 nearby spiral galaxies
Published in Monthly notices of the Royal Astronomical Society (28-10-2021)“…ABSTRACT The feedback from young stars (i.e. pre-supernova) is thought to play a crucial role in molecular cloud destruction. In this paper, we assess the…”
Get full text
Journal Article -
6
Dense molecular gas properties on 100 pc scales across the disc of NGC 3627
Published in Monthly notices of the Royal Astronomical Society (01-09-2021)“…ABSTRACT It is still poorly constrained how the densest phase of the interstellar medium varies across galactic environment. A large observing time is required…”
Get full text
Journal Article -
7
HERSCHEL FAR-INFRARED AND SUBMILLIMETER PHOTOMETRY FOR THE KINGFISH SAMPLE OF NEARBY GALAXIES
Published in The Astrophysical journal (20-01-2012)“…New far-infrared and submillimeter photometry from the Herschel Space Observatory is presented for 61 nearby galaxies from the Key Insights on Nearby Galaxies:…”
Get full text
Journal Article -
8
Erratum: “Mapping Metallicity Variations across Nearby Galaxy Disks” (2019, ApJ, 887, 80)
Published in The Astrophysical journal (17-05-2021)Get full text
Journal Article -
9
A STUDY OF HEATING AND COOLING OF THE ISM IN NGC 1097 WITH HERSCHEL-PACS AND SPITZER-IRS
Published in The Astrophysical journal (01-06-2012)“…NGC 1097 is a nearby Seyfert 1 galaxy with a bright circumnuclear starburst ring, a strong large-scale bar, and an active nucleus. We present a detailed study…”
Get full text
Journal Article -
10
A sensitive, high-resolution, wide-field IRAM NOEMA CO(1-0) survey of the very nearby spiral galaxy IC 342
Published 10-10-2023“…A&A 680, A4 (2023) We present a new wide-field 10.75 x 10.75 arcmin^2 (~11x11 kpc^2), high-resolution (theta = 3.6" ~ 60 pc) NOEMA CO(1-0) survey of the very…”
Get full text
Journal Article -
11
Investigating the link between inner gravitational potential and star-formation quenching in CALIFA galaxies
Published 08-07-2022“…A&A 665, A90 (2022) It has been suggested that the gravitational potential can have a significant role in suppressing the star formation in the nearby…”
Get full text
Journal Article -
12
Quantifying the energetics of molecular superbubbles in PHANGS galaxies
Published 14-06-2023“…A&A 676, A67 (2023) Star formation and stellar feedback are interlinked processes that redistribute energy and matter throughout galaxies. When young, massive…”
Get full text
Journal Article -
13
[C II] 158 μm EMISSION AS A STAR FORMATION TRACER
Published in The Astrophysical journal (10-02-2015)“…The [CII] 157.74 mu m transition is the dominant coolant of the neutral interstellar gas, and has great potential as a star formation rate (SFR) tracer. Using…”
Get full text
Journal Article -
14
THE PdBI ARCSECOND WHIRLPOOL SURVEY (PAWS): ENVIRONMENTAL DEPENDENCE OF GIANT MOLECULAR CLOUD PROPERTIES IN M51
Published in The Astrophysical journal (20-03-2014)“…Using data from the PdBI Arcsecond Whirlpool Survey (PAWS), we have generated the largest extragalactic giant molecular cloud (GMC) catalog to date, containing…”
Get full text
Journal Article -
15
Dense Gas in a Giant Molecular Filament
Published 22-06-2020“…A&A 641, A53 (2020) Recent surveys of the Galactic plane in the dust continuum and CO emission lines reveal that large ($\gtrsim 50$~pc) and massive ($\gtrsim…”
Get full text
Journal Article -
16
ALMA Resolves Giant Molecular Clouds in a Tidal Dwarf Galaxy
Published 02-11-2020“…A&A 645, A97 (2021) Tidal dwarf galaxies (TDGs) are gravitationally bound condensations of gas and stars formed during galaxy interactions. Here we present…”
Get full text
Journal Article -
17
Comparing the pre-SNe feedback and environmental pressures for 6000 HII regions across 19 nearby spiral galaxies
Published 25-10-2021“…The feedback from young stars (i.e. pre-supernova) is thought to play a crucial role in molecular cloud destruction. In this paper, we assess the feedback…”
Get full text
Journal Article -
18
Dense molecular gas properties on 100 pc scales across the disc of NGC 3627
Published 17-06-2021“…It is still poorly constrained how the densest phase of the interstellar medium varies across galactic environment. A large observing time is required to…”
Get full text
Journal Article -
19
THE PdBI ARCSECOND WHIRLPOOL SURVEY (PAWS): MULTI-PHASE COLD GAS KINEMATIC OF M51
Published in The Astrophysical journal (20-03-2014)“…The kinematic complexity and the favorable position of M51 on the sky make this galaxy an ideal target to test different theories of spiral arm dynamics. Using…”
Get full text
Journal Article -
20
Ubiquitous velocity fluctuations throughout the molecular interstellar medium
Published 03-07-2020“…The density structure of the interstellar medium (ISM) determines where stars form and release energy, momentum, and heavy elements, driving galaxy evolution…”
Get full text
Journal Article