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#InterstellarMedium

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Posts tagged #InterstellarMedium

VizieR J/A+A/707/A20

New in the #VirtualObservatory: “NGC 1068 vel.-int. intensities and luminosities” by Lin S. et al.
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/707/A20
#ActiveGalacticNuclei #InterstellarMedium #MillimeterAstronomy #SubmillimeterAstronomy

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VizieR J/A+A/706/A85

New in the #VirtualObservatory: “Size-Shape Difference for 67 GASP galaxies” by Lassen A.E. et al.
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/706/A85
#InterstellarMedium #Spectroscopy #Redshifted #Galaxies

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VizieR J/A+A/706/A40

New in the #VirtualObservatory: “PHANGS-JWST GMC catalog” by Bazzi Z. et al.
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/706/A40
#InfraredPhotometry #MolecularClouds #Galaxies #InterstellarMedium

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VizieR J/MNRAS/542/52

New in the #VirtualObservatory: “3D velocities of YSO-MC associations” by Zhou J.-X. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/542/...
#MolecularClouds #YoungStellarObjects #InterstellarMedium

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VizieR J/A+A/703/A103

New in the #VirtualObservatory: “PAHs in star-forming regions” by Egorov O.V. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/703/A1...
#InterstellarMedium #HIiRegions #InfraredPhotometry #Galaxies

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VizieR J/ApJ/953/104

New in the #VirtualObservatory: “YSOs from Spitzer & Herschel surveys in LMC” by Kokusho T. et al.
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/953/104
#Extinction #Surveys #InterstellarMedium #MagellanicClouds

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VizieR J/A+A/702/A23

New in the #VirtualObservatory: “TMC-1 analysis of C and S isotopologues” by Fuentetaja R. et al.
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/702/A23
#RadioAstronomy #Spectroscopy #InterstellarMedium

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VizieR J/MNRAS/532/4661

New in the #VirtualObservatory: “178 dense cores study with HGBS of TMC1 -II” by Kirk J.M. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/532/...
#InterstellarMedium #Photometry #Spectroscopy #YoungStellarObjects

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VizieR J/A+A/701/A111

New in the #VirtualObservatory: “PDRs4All XVI. Orion Bar template spectra” by Van De Putte D. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/701/A1...
#InfraredSources #Nebulae #InterstellarMedium #Spectroscopy

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VizieR J/A+A/700/A238

New in the #VirtualObservatory: “Line list for minor acetylene isotopologs” by Lee M. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/700/A2...
#InterstellarMedium #AtomicPhysics #InfraredAstronomy #Spectroscopy

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VizieR J/A+A/700/A158

New in the #VirtualObservatory: “NGC 7023 and Horsehead line list and spectra” by Misselt K. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/700/A1...
#MolecularClouds #Extinction #InterstellarMedium #Spectroscopy

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An "Encounter" With Something From Outside Our Solar System May Have Cooled Earth In A Big Way It's possible our movement through the galaxy may affect our climate.

#mwgic #2025 #Climate #InterstellarMedium #Heliosphere #InterstellarDustClouds

Global cooling due to clouds of interstellar dust? May have happened in the past, may happen in the future.

www.iflscience.com/an-encounter...

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VizieR J/A+A/699/A346

New in the #VirtualObservatory: “Gas and dust in DustPedia galaxies” by Salvestrini F. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/699/A3...
#Galaxies #InterstellarMedium

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VizieR J/ApJS/276/15

New in the #VirtualObservatory: “Compilation of optical starlight polarization” by Panopoulou G.V. et al.
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/276/15
#MagneticFields #InterstellarMedium #Polarimetry

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Know your solar system...

#solarsystem #sun #ortcloud #interstellarmedium #planets #unify

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The GHOSDT Simulations: II. Missing Molecules in Simulations of a
Self-Regulated Interstellar Medium
Alon Gurman, Amiel Sternberg et al.
Paper
Details
#GHOSDTSimulations #InterstellarMedium #AstrophysicsResearch

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Tracking Molecules In the Interstellar Medium Stars don’t form out of nothing, but tracking the gas and dust that do eventually form stars is hard. They float around the galaxy at almost absolute zero, emitting essentially no light, and generally...

Tracking Molecules In the Interstellar Medium #Science #Space #Astrophysics #InterstellarMedium #MolecularResearch

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VizieR J/AJ/168/203

New in the #VirtualObservatory: “Dust clouds masses, color excesses and distances” by Sun M. et al.
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/168/203
#Extinction #InterstellarMedium #VisibleAstronomy #RadioSources

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Stunning color-coded map of the Milky Way's magnetic field, created by the Planck satellite. The image reveals the strength of the field in the central disk, appearing as swirling blue and orange hues.  This visualization highlights the complex interplay of charged gas and magnetism in our galaxy.

Stunning color-coded map of the Milky Way's magnetic field, created by the Planck satellite. The image reveals the strength of the field in the central disk, appearing as swirling blue and orange hues. This visualization highlights the complex interplay of charged gas and magnetism in our galaxy.

Astronomy Picture from 27/01/2015

Our Galaxy's Magnetic Field from Planck

Source: https://apod.nasa.gov/apod/ap150127.html


#MilkyWayMagneticField #PlanckSatellite #GalacticMagnetism #SpaceScience #AstronomyImage #CosmicBeauty #InterstellarMedium #Astrophysics #GalaxyMap #ScienceImage

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Image of Henize 70, a luminous superbubble in the Large Magellanic Cloud (LMC). This 300-lightyear-diameter ring-shaped nebula is formed by winds from massive stars and supernova explosions.  The image shows the superbubble's intricate structure within a backdrop of countless stars. The vibrant pink hues highlight the expanding hot gas within.

Image of Henize 70, a luminous superbubble in the Large Magellanic Cloud (LMC). This 300-lightyear-diameter ring-shaped nebula is formed by winds from massive stars and supernova explosions. The image shows the superbubble's intricate structure within a backdrop of countless stars. The vibrant pink hues highlight the expanding hot gas within.

Astronomy Picture from 13/06/1998

Henize 70: A SuperBubble In The LMC

Source: https://apod.nasa.gov/apod/ap980613.html


#Henize70 #Superbubble #LMC #LargeMagellanicCloud #Stars #Nebula #Astronomy #Space #Cosmology #GalaxyEvolution #Supernova #InterstellarMedium #Astrophysics

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- rays with a form of #electromagnetic radiation called the interstellar radiation field.

The 3 distinguishing areas within the #InterstellarMedium are the forms of matter that include molecular, ionic & atomic types.

The density of the matter & its temperature are also part of this unique medium.

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A full-sky image from ESA's Planck satellite reveals the Milky Way's magnetic field structure.  Curvy lines depict the magnetic field, with dark red indicating the galactic plane.  Arches above the plane are likely remnants of past explosions.  The image highlights the role of magnetic fields in shaping the interstellar medium and influencing star formation.

A full-sky image from ESA's Planck satellite reveals the Milky Way's magnetic field structure. Curvy lines depict the magnetic field, with dark red indicating the galactic plane. Arches above the plane are likely remnants of past explosions. The image highlights the role of magnetic fields in shaping the interstellar medium and influencing star formation.

Astronomy Picture from 17/06/2020

Magnetic Streamlines of the Milky Way

Source: https://apod.nasa.gov/apod/ap200617.html


#MilkyWayMagnetism #InterstellarMedium #PlanckSatellite #CosmicMagneticFields #SpaceScience #Astronomy #Astrophysics #GalaxyEvolution #StarFormation #MagneticFields

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A stunning image of runaway star HD 77581, creating a bow shock as it travels through interstellar space at over 50 miles per second.  The bright star at the center is saturated, showing diffraction spikes.  A faint, arcing bow wave of compressed gas is visible, a result of the star's rapid movement. The image hints at the star's origin, linked to a supernova explosion and its companion X-ray pulsar, Vela X-1.

A stunning image of runaway star HD 77581, creating a bow shock as it travels through interstellar space at over 50 miles per second. The bright star at the center is saturated, showing diffraction spikes. A faint, arcing bow wave of compressed gas is visible, a result of the star's rapid movement. The image hints at the star's origin, linked to a supernova explosion and its companion X-ray pulsar, Vela X-1.

Astronomy Picture from 03/12/1997

Runaway Star

Source: https://apod.nasa.gov/apod/ap971203.html


#RunawayStar #HD77581 #BowShock #InterstellarMedium #SupernovaRemnant #VelaConstellation #Astronomy #Astrophysics #Space #Cosmos #Stars #Pulsar #VelaX1

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Stunning infrared image of the Milky Way's dust tapestry, revealing intricate filamentary structures within 500 light-years of Earth.  Red depicts gas at 10 Kelvin, white at 40 Kelvin. The pink band is warm gas in the galactic plane. Bright regions show dense molecular clouds forming stars; dimmer areas are diffuse interstellar gas and dust.  This image combines data from the Planck and IRAS satellites, providing insight into our galaxy's history and star formation.

Stunning infrared image of the Milky Way's dust tapestry, revealing intricate filamentary structures within 500 light-years of Earth. Red depicts gas at 10 Kelvin, white at 40 Kelvin. The pink band is warm gas in the galactic plane. Bright regions show dense molecular clouds forming stars; dimmer areas are diffuse interstellar gas and dust. This image combines data from the Planck and IRAS satellites, providing insight into our galaxy's history and star formation.

Astronomy Picture from 22/03/2010

The Nearby Milky Way in Cold Dust

Source: https://apod.nasa.gov/apod/ap100322.html


#MilkyWay #CosmicDust #InfraredAstronomy #PlanckSatellite #StarFormation #InterstellarMedium #SpaceExploration #GalaxyEvolution #AstronomyImage #Astrophysics

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A stunning telescopic view of Gamma Cassiopeiae, a bright star interacting with the ghostly interstellar clouds IC 59 and IC 63 in the constellation Cassiopeia. The image showcases the vibrant red H-alpha emission of IC 63 and the bluish reflection nebula of IC 59, highlighting the star's powerful influence on these nearby cosmic clouds, approximately 600 light-years away.  The cosmic scene spans over 10 light-years.

A stunning telescopic view of Gamma Cassiopeiae, a bright star interacting with the ghostly interstellar clouds IC 59 and IC 63 in the constellation Cassiopeia. The image showcases the vibrant red H-alpha emission of IC 63 and the bluish reflection nebula of IC 59, highlighting the star's powerful influence on these nearby cosmic clouds, approximately 600 light-years away. The cosmic scene spans over 10 light-years.

Astronomy Picture from 28/10/2023

The Ghosts of Gamma Cas

Source: https://apod.nasa.gov/apod/ap231028.html


#GammaCassiopeiae #IC59 #IC63 #Nebula #Astrophotography #DeepSpace #Space #Astronomy #Stars #ConstellationCassiopeia #CosmicClouds #Halpha #InterstellarMedium

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False-color image of an all-sky HI (neutral hydrogen) survey. The bright band across the center represents the plane of our Milky Way galaxy, showing vast clouds of hydrogen gas tens to hundreds of light-years across.  These structures are shaped by stellar activity within the galactic disk.  The image is based on radio wave emissions from hydrogen atoms at a wavelength of 21 centimeters.

False-color image of an all-sky HI (neutral hydrogen) survey. The bright band across the center represents the plane of our Milky Way galaxy, showing vast clouds of hydrogen gas tens to hundreds of light-years across. These structures are shaped by stellar activity within the galactic disk. The image is based on radio wave emissions from hydrogen atoms at a wavelength of 21 centimeters.

Astronomy Picture from 13/01/2001

A Sky Full Of Hydrogen

Source: https://apod.nasa.gov/apod/ap010113.html


#HI21cm #RadioAstronomy #MilkyWay #InterstellarMedium #NeutralHydrogen #SpaceGas #AstronomyImage #Astrophysics #GalaxyMap #AllSkySurvey

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Image of runaway star HD 77581, a bright star creating a bow shock wave as it travels through interstellar space.  The star is over-exposed creating a spiky cross shape in the center of the image. A faint arc of compressed gas is visible behind it. This is likely due to the supernova explosion of its companion star, Vela X-1, a pulsar.

Image of runaway star HD 77581, a bright star creating a bow shock wave as it travels through interstellar space. The star is over-exposed creating a spiky cross shape in the center of the image. A faint arc of compressed gas is visible behind it. This is likely due to the supernova explosion of its companion star, Vela X-1, a pulsar.

Astronomy Picture from 27/11/1999

Runaway Star

Source: https://apod.nasa.gov/apod/ap991127.html


#RunawayStar #HD77581 #BowShock #InterstellarMedium #SupernovaRemnant #VelaConstellation #Astronomy #Astrophysics #Space #Cosmology #Stars #Pulsar #VelaX1

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Stunning infrared image of runaway star Zeta Ophiuchi creating a dramatic bow shock as it plows through interstellar dust and gas. The vibrant red and green colors highlight the compressed and heated material, showcasing the star's powerful stellar wind.  Zeta Ophiuchi, 20 times more massive than our sun, was likely ejected from a binary system after its companion exploded as a supernova.  This image spans 12 light-years.

Stunning infrared image of runaway star Zeta Ophiuchi creating a dramatic bow shock as it plows through interstellar dust and gas. The vibrant red and green colors highlight the compressed and heated material, showcasing the star's powerful stellar wind. Zeta Ophiuchi, 20 times more massive than our sun, was likely ejected from a binary system after its companion exploded as a supernova. This image spans 12 light-years.

Astronomy Picture from 05/07/2015

Zeta Oph: Runaway Star

Source: https://apod.nasa.gov/apod/ap150705.html


#ZetaOphiuchi #RunawayStar #BowShock #InterstellarMedium #InfraredAstronomy #Space #Astronomy #Astrophysics #Cosmology #Stars #Nebula #SpitzerSpaceTelescope #NASA

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A diagram illustrating the Sun's movement through the Local Interstellar Cloud, a region of mostly hydrogen gas within the Milky Way galaxy. The diagram shows the Sun's trajectory and the relative positions of nearby stars like Sirius, Alpha Centauri, Procyon and Altair, within a 10 light-year radius.  The cloud's motion is indicated, along with the direction of the Sun's movement towards the galactic center.  The image highlights the complex structure and dynamics of the interstellar medium.

A diagram illustrating the Sun's movement through the Local Interstellar Cloud, a region of mostly hydrogen gas within the Milky Way galaxy. The diagram shows the Sun's trajectory and the relative positions of nearby stars like Sirius, Alpha Centauri, Procyon and Altair, within a 10 light-year radius. The cloud's motion is indicated, along with the direction of the Sun's movement towards the galactic center. The image highlights the complex structure and dynamics of the interstellar medium.

Astronomy Picture from 11/04/2000

The Local Interstellar Cloud

Source: https://apod.nasa.gov/apod/ap000411.html


#LocalInterstellarCloud #InterstellarMedium #MilkyWay #SolarNeighborhood #SpaceExploration #Astronomy #Astrophysics #Sun'sJourney #Stars #Galaxy

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Illustration depicting the Sun's journey through the Local Interstellar Cloud (Local Fluff), a region of the interstellar medium within 20 light-years.  The image shows the Sun's direction of motion, its location relative to nearby stars (like Sirius and Alpha Centauri), and the flow of interstellar gas.  Data from the IBEX satellite contributed to creating this map of our solar neighborhood.

Illustration depicting the Sun's journey through the Local Interstellar Cloud (Local Fluff), a region of the interstellar medium within 20 light-years. The image shows the Sun's direction of motion, its location relative to nearby stars (like Sirius and Alpha Centauri), and the flow of interstellar gas. Data from the IBEX satellite contributed to creating this map of our solar neighborhood.

Astronomy Picture from 22/12/2024

The Local Fluff

Source: https://apod.nasa.gov/apod/ap241222.html


#LocalInterstellarCloud #MilkyWay #ISM #Sun #IBEX #Astrophysics #Space #Astronomy #Stars #SolarSystem #LocalFluff #InterstellarMedium #APOD

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