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- 01GKMJ8Q1DAP5BRHGE8SX8FTSP classification A1.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP date "2023".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP language "eng".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP type journalArticle.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP hasPart 01GWRTV3DHDCWP3Q78QB49D6Y3.pdf.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP subject "Physics and Astronomy".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP doi "10.3847/2041-8213/aca90a".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP issn "2041-8205".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP issn "2041-8213".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP issue "2".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP volume "944".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP abstract "The earliest stages of star formation, when young stars are still deeply embedded in their natal clouds, represent a critical phase in the matter cycle between gas clouds and young stellar regions. Until now, the high-resolution infrared observations required for characterizing this heavily obscured phase (during which massive stars have formed, but optical emission is not detected) could only be obtained for a handful of the most nearby galaxies. One of the main hurdles has been the limited angular resolution of the Spitzer Space Telescope. With the revolutionary capabilities of the James Webb Space Telescope (JWST), it is now possible to investigate the matter cycle during the earliest phases of star formation as a function of the galactic environment. In this Letter, we demonstrate this by measuring the duration of the embedded phase of star formation and the implied time over which molecular clouds remain inert in the galaxy NGC 628 at a distance of 9.8 Mpc, demonstrating that the cosmic volume where this measurement can be made has increased by a factor of > 100 compared to Spitzer. We show that young massive stars remain embedded for 5.1(-1.4)(+2.7) Myr (2.3(-1.4)(+2.7) Myr of which being heavily obscured), representing similar to 20% of the total cloud lifetime. These values are in broad agreement with previous measurements in five nearby (D < 3.5 Mpc) galaxies and constitute a proof of concept for the systematic characterization of the early phase of star formation across the nearby galaxy population with the PHANGS-JWST survey.".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author D7B9D050-F5BD-11E8-8ADC-2DCE5607D3EF.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:03bad018-5c37-468e-94d7-2415dfd144b4.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:09a79c75-5e30-4d87-8ec7-6acd43ea75cf.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:1cbf6313-870f-4fa5-b4d5-6dec177c1c04.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:24b22642-899e-4a7e-9343-eedaada5c9f9.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:314c5ec8-f5e1-40f8-b4d8-95f01e72d1ab.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:35e125a8-8c63-492f-b819-5631f61b2040.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:37b7c0b8-9d4e-49e3-96a2-752ddb4ac254.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:3af9ade1-d923-45b9-94e2-6840860ff26d.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:438bad33-dcf9-4456-ab03-b94b5c1592d8.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:4dc4baa9-4835-4648-ba44-9b4dec9970d1.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:529fd8cb-4da7-409c-8b5d-98aa41923feb.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:6d1f2dfc-3887-41f1-af2e-605e3684c5e9.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:7617f1c5-0d92-41e1-862d-a813834f6cd1.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:7a2ca004-48b4-41b2-8c3f-3bf035a266e7.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:890a411c-12e1-40fc-b2ea-3295a14812be.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:8d8e8eee-7d92-47c4-ada7-f084dd7ede8e.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:9815cd39-9ea1-4b6e-856e-c74700a671e3.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:9bcaa6dc-9671-4109-8446-926994bad55f.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:9eeb34f8-bfd7-40f4-8532-4c10f83f9cd9.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:ac779d79-72e0-4bc3-a7f6-5a7d41333305.
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- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:bd0b6a98-873c-49e8-b0ae-2fd5d91d7adc.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:c88aa4bc-c846-44cd-928a-2938112b0c51.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:dbe956f9-9a9f-4660-b584-720682ae7429.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:de56275d-74f2-4de6-a315-97602d32ea8e.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:e41d30fc-b24a-4316-8a40-17086bc0dccf.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:e44b4c58-c1ae-42b9-8631-7c9c20eb9d4e.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:e5b8161d-c017-403c-afb7-ea9ca4296454.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:e65c87c9-7eb1-4668-88d5-b1e2e38d3519.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:f917108b-3436-4acc-9809-42f1e2f9e85f.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:fb33154c-64a1-4ec1-9293-f5fd7c1b9596.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:fe1a8a42-1887-4868-a09e-7509b2ad0caa.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP author urn:uuid:ffe497b3-21ab-41b8-9548-b8256d1e9ce8.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP dateCreated "2022-12-06T20:33:05Z".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP dateModified "2024-12-12T10:20:12Z".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP name "PHANGS-JWST first results : duration of the early phase of massive star formation in NGC628".
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP pagination urn:uuid:1d8d1dbb-7cc4-4199-927b-8760b26b3f7d.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP sameAs LU-01GKMJ8Q1DAP5BRHGE8SX8FTSP.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP sourceOrganization urn:uuid:e03e0959-188b-4545-bb2b-09429eeab3cd.
- 01GKMJ8Q1DAP5BRHGE8SX8FTSP type A1.