Published 2020 | Version v1
Journal article

Dust evolution in pre-stellar cores

  • 1. LERMA & UMR8112 du CNRS, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC University Paris 06, F-75014 Paris (France)
  • 2. Institut de Radioastronomie Millimétrique (IRAM), 300 rue de la Piscine, 38400 Saint-Martin d'Hères (France)
  • 3. Instituto de Radioastronomía Milimétrica, IRAM, Avenida Divina Pastora 7, Local 20, E-18012, Granada (Spain)
  • 4. Sterrenkundig Instituut Anton Pannekoek, University of Amsterdam, Science Park 904, 1098 XH Amsterdam (Netherlands)
  • 5. Institute of Astronomy and Astrophysics, Academia Sinica, Astronomy–Mathematics Building, AS/NTU, No.1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan (China)

Description

Dust grains are the building blocks of future planets. They evolve in size, shape and composition during the life cycle of the interstellar medium. We seek to understand the process which leads from diffuse medium grains to dust grains in the vicinity of protostars inside disks. As a first step, we propose to characterize the dust evolution inside pre-stellar cores thanks to multi-wavelength observations. We will present how NIKA2 maps are crucial to better constrain dust properties and we will introduce SIGMA: a new flexible dust model in open access.

Availability note (English)

Available from https://www.epj-conferences.org/articles/epjconf/pdf/2020/04/epjconf_mmuniverse2019_00013.pdf; https://doaj.org/article/eb84aca7b61d4dd4ac0d620303b432d8

Additional details

Publishing Information

Journal Title
EPJ. Web of Conferences
Journal Volume
228
Journal Page Range
vp.
ISSN
2100-014X

Conference

Title
1. mm Universe @ NIKA2 workshop - Observing the mm Universe with the NIKA2 Camera
Dates
3-7 Jun 2019
Place
Grenoble (France)

INIS

Country of Publication
France
Country of Input or Organization
France
INIS RN
53116043
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
DUSTS; LIFE CYCLE; PLANETS; PROTOSTARS; SHAPE; WAVELENGTHS