Josep Martí

Dr. Josep Martí


Research Focus & Metrics

Academic Career Length

35Years (1992-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 March 2013 in Astroparticle Physics
Verified
Journal Article
Closed access
BAB.S. Acharya
B.S. Acharya
MAM. Actis
M. Actis
TAT. Aghajani
T. Aghajani
GAG. Agnetta
G. Agnetta
JAJ. Aguilar
J. Aguilar
PŻP. Żychowski
P. Żychowski

11 December 2005 in Monthly Notices of the Royal Astronomical Society
Verified
Journal Article
Closed access
PDF file
JCJorge Casares
Jorge Casares
MRM. Ribo
M. Ribo
IRI. Ribas
I. Ribas
JPJ. M. Paredes
J. M. Paredes
JMJosep Martí
Josep Martí
AHA. Herrero
A. Herrero

26 November 2010 in Science
Verified
Journal Article
Closed access
PDF file
CCCarlos Carrasco-González
Carlos Carrasco-González
LRLuis F. Rodríguez
Luis F. Rodríguez
GAGuillem Anglada
Guillem Anglada
JMJosep Martí
Josep Martí
JTJosé M. Torrelles
José M. Torrelles
MOMayra Osorio
Mayra Osorio
Stellar Jets: Supersonic jets of energized charged particles are a common phenomenon in astrophysics, emanating from sources that range widely in mass: from brown dwarfs to super massive black holes in the centers of galaxies. Carrasco-González et al. (p. 1209 ; see the Perspective by Ray ) present observations, of a jet emanating from a young stellar object, which show that the jet is magnetized and has characteristics that are similar to those of jets found in much larger and more massive systems. The results support the idea that all astrophysical jets are launched and collimated through the same basic mechanism, involving launching of material along magnetic field lines.

1 September 2012 in Publications of the Astronomical Society of the Pacific
Verified
Journal Article
Open access
MHM. G. Hoare
M. G. Hoare
CPCormac Purcell
Cormac Purcell
ECE. B. Churchwell
E. B. Churchwell
PDP. Diamond
P. Diamond
WCW. D. Cotton
W. D. Cotton
AZAlbert Zijlstra
Albert Zijlstra
We describe the motivation, design, and implementation of the CORNISH survey, an arcsecondresolution radio continuum survey of the inner galactic plane at 5 GHz using the Very Large Array (VLA). It is a blind survey coordinated with the northern Spitzer GLIMPSE I region covering 10\ub0 < l < 65\ub0 and |b| < 1\ub0 at similar resolution. We discuss in detail the strategy that we employed to control the shape of the synthesised beam across this survey, which covers a wide range of fairly low declinations. Two snapshots separated by 4 h kept the beam elongation to less that 1.5 over 75% of the survey area and less than 2 over 98% of the survey. The prime scientific motivation is to provide an unbiased survey for ultra-compact H II regions to study this key phase in massive star formation. A sensitivity around 2 mJy will allow the automatic distinction between radio-loud and radio-quiet mid- IR sources found in the Spitzer surveys. This survey has many legacy applications beyond star formation, including evolved stars, active stars and binaries, and extragalactic sources. The CORNISH survey for compact ionized sources complements other Galactic plane surveys that target diffuse and nonthermal sources, as well as atomic and molecular phases to build up a complete picture of the interstellar medium in the Galaxy.Peer reviewed: YesNRC publication: Ye

20 February 2013 in The Astrophysical Journal Supplement Series
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Journal Article
Open access
CPCormac Purcell
Cormac Purcell
MHM. G. Hoare
M. G. Hoare
WCW. D. Cotton
W. D. Cotton
SLS. L. Lumsden
S. L. Lumsden
JUJ. S. Urquhart
J. S. Urquhart
AZAlbert Zijlstra
Albert Zijlstra

1 October 1993 in The Astrophysical Journal
Verified
Journal Article
Closed access
JMJosep Martí
Josep Martí
LRL. F. Rodriguez
L. F. Rodriguez
BRB. Reipurth
B. Reipurth