NANOCOSMOS at the Guillermo Haro School on Molecular Astrophysics (Puebla, Mexico)

Prof. José Cernicharo has been awarded with the Guillermo Haro Visiting Professorship 2016 at the Instituto Nacional de Astrofísica, Óptica y Electrónica (INAOE, posterGH16Puebla, Mexico). Following this award, INAOE has organized the Guillermo Haro School on Molecular Astrophysics (October 11 – 21, 2016). Several NANOCOSMOS scientists (Asunción Fuente from CNIG-IGN, Nuria Marcelino, José Pablo Fonfría and Luis Velilla from ICMM-CSIC) will give lectures on the following topics:

  • Molecular Astrophysics, Spectroscopy, Chemistry in the ISM (José Cernicharo)
  • Physical and chemical processes in the ISM, Protoplanetary disks (Asunción Fuente)
  • Observational methods and interpretation (Nuria Marcelino)
  • Molecular excitation and radiative transfer, Circumstellar medium (José Pablo Fonfría)
  • Chemistry in the circumstellar medium, atmospheric  effects and calibration (Luis Velilla)

José Cernicharo will give a public talk in Puebla downtown on Thursday 13: “Moléculas en el espacio: Astroquímica”.

ECLA 2016 – webpage open

Ecla2016-1125x510

The second announcement of the European Conference on Laboratory Astrophysics – “Gas on the Rocks” – ECLA 2016 has been issued today.  This conference will be held at the CSIC headquarters (Madrid, Spain) in November 21 – 25, 2016. The webpage is open with all the relevant information.

www.ecla2016.com

More than 30 invited researchers will address new insights on the following science topics:

  • Comets, asteroids, meteorites and the primitive Solar System nebula: formation and evolution
  • Protoplanetary disks and planet formation
  • Planet, Moon, and exoplanet surfaces and atmospheres
  • The signatures of the evolving interstellar medium
  • Dense Clouds: the gas-ice interface and molecular complexity
  • Chemical fingerprints of star formation
  • The late stages of star evolution: dust formation
  • Supernovae and shocks: high-energy processing of matter

NANOCOSMOS will organize the ECLA2016 – Gas on the Rocks conference

Stardustiram_PdV

The European Conference on Laboratory Astrophysics – Gas on the Rocks (ECLA2016) will be held at the CSIC headquarters in Madrid on November 21 – 25, 2016.

The conference will address the state of the art in laboratory astrophysics within the context of new astrophysical data and to improve communication and collaboration between astrophysicists, physicists and (geo) chemists. Hence, the conference structure will consist of invited talks presenting topics in astrophysics and planetary science and related laboratory astrophysics activities. Contributing talks will be selected to complement the topics from the astrophysical, laboratory, and theoretical/modeling points of view.

More info here

 

NANOCOSMOS workshops/meetings

2017

NANOCOSMOS Interstellar Dust Meeting

Date: 12 – 13 June 2017

Place: Université Paul Sabatier (Toulouse, France)

Key dates: 

Abstract submission deadline: April 30th, 2017

Registration deadline: May 14th, 2017

Webpage: https://epolm3-nanocosm.sciencesconf.org/

2016

European Conference on Laboratory AstrophysicsGas on the Rocks (ECLA2016)

Outcome of the conference: See “A summary of the ECLA2016” link

November 21 – 25, 2016 (CSIC Headquarters, Madrid, Spain)

Webpage: ECLA2016

FIRST ANNOUNCEMENT

Key dates:
Second announcement:  February 1st, 2016 (opening of the conference web page).
Deadline for abstract submission: June 15, 2016
Deadline for early registration: July 15, 2016
Deadline for information participants about selected contributing talks: June 30, 2016
Final program: July 15, 2016
Last announcement with final details: November 1st, 2016

Motivation:

Over the last decade, European research activities in the field of laboratory astrophysics have experienced an impressive increase in their potential to address astrophysical problems, in particular by providing essential information on the physical and chemical processes leading to chemical complexity in space resulting in star and planet formation. These activities have been motivated by the interpretation of astronomical observations obtained with single dish telescopes and short baseline interferometers. The wealth of data obtained with ALMA, space facilities (Herschel, Spitzer, Rosetta, the coming JWST, E-ELT), and other ground based observatories (VLTI, NOEMA, …), require new methodologies for the astrophysical modeling that will lead to new challenges for laboratory astrophysics.

This conference aims to address the state of the art in laboratory astrophysics within the context of these new astrophysical data and to improve communication and collaboration between astrophysicists, physicists and (geo) chemists. Hence, the conference structure will consist of invited talks presenting topics in astrophysics and planetary science and related laboratory astrophysics activities. Contributing talks will be selected to complement the topics from the astrophysical, laboratory, and theoretical/modeling points of view.

The astrophysical areas that will be addressed are:

Comets, asteroids, meteorites and the primitive Solar System nebula: formation and evolution
Protoplanetary disks and planet formation
Planet, Moon, and exoplanet surfaces and atmospheres
The signatures of the evolving interstellar medium
Dense Clouds: the gas-ice interface
Chemical fingerprints of star formation
The late stages of star evolution: dust formation
Supernovae and shocks: high-energy processing of matter

The conference will cover studies in many fields such as spectroscopy, analytical (geo) chemistry, reactivity, nanoscience, and quantum chemistry, pertaining to different matter components (gas, plasma, PAHs, ices, dust, solid surfaces, …).

SOC composition
Jose Cernicharo (chair). ICMM-CSIC, Madrid, Spain
Christine Joblin (co-chair). IRAP, Univ. Paul Sabatier/CNRS, Toulouse, France
Isabel Tanarro. IEM-CSIC, Madrid, Spain
Jose Angel Martín Gago. ICMM-CSIC, Madrid, Spain
Karine Demyk. IRAP, Univ. Paul Sabatier/CNRS, Toulouse, France
Jean-Hugues Fillion. LERMA, UPCM Univ.  Paris 06, & Obs. Paris, France
Maria Elisabetta Palumbo. INAF-Catania Astrophysical Obs., Italy
André Canosa. IPR, Univ. Rennes 1/CNRS, France
Harold Linnartz. Leiden Obs., Univ. of Leiden, The Netherlands
Liv Hornekaer. iNANO, Aarhus Univ., Danemark
Peter Sarre. School of Chemistry, Nottingham Univ., UK
Stephan Schlemmer. Phys. Inst., Univ. Koln, Germany
Jonathan Tennyson. Univ. College London, UK
Yves Marrochi. CRPG-CNRS, Nancy, France
Guillermo Muñoz Caro. CAB, INTA-CSIC, Madrid, Spain

LOC composition
Isabel Tanarro (Chair). IEM-CSIC, Madrid, Spain
Belén Maté. IEM-CSIC, Madrid, Spain
Víctor J. Herrero. IEM-CSIC, Madrid, Spain
José Luis Doménech. IEM-CSIC, Madrid, Spain
Ángel González-Valdenebro. IEM-CSIC, Madrid, Spain
Marcelo Castellanos (co-chair). ICMM-CSIC, Madrid, Spain
Belén Tercero.  ICMM-CSIC, Madrid, Spain
Juan Ramón Pardo. ICMM-CSIC, Madrid, Spain
Juan Antonio Corbalán. ICMM-CSIC, Madrid, Spain
Natalia Ruiz-Zelmanovich. ICMM-CSIC, Madrid, Spain

The project

idea

Cosmic dust is made in evolved stars. However, the processes involved in the formation and evolution of dust remain so far unknown. NANOCOSMOS will take advantage of the new observational capabilities (increased angular resolution) of the Atacama Large Millimeter/submillimeter Array (ALMA) to unveil the physical and chemical conditions in the dust formation zone of evolved stars. These observations in combination with novel top-level ultra-high vacuum experiments and astrophysical modelling will provide a cutting-edge view of cosmic dust.