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Dive into the research topics where Sergio Martin is active.

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Featured researches published by Sergio Martin.


The Astrophysical Journal | 2014

Suppression of Star Formation in NGC 1266

Katherine Alatalo; Mark D. Lacy; Lauranne Lanz; T. Bitsakis; Philip N. Appleton; Kristina Nyland; Sabrina L. Cales; Philip Chang; Timothy A. Davis; P. T. de Zeeuw; Carol J. Lonsdale; Sergio Martin; David S. Meier; P. Ogle

NGC1266 is a nearby lenticular galaxy that harbors a massive outflow of molecular gas powered by the mechanical energy of an active galactic nucleus (AGN). It has been speculated that such outflows hinder star formation (SF) in their host galaxies, providing a form of feedback to the process of galaxy formation. Previous studies, however, indicated that only jets from extremely rare, high power quasars or radio galaxies could impart significant feedback on their hosts. Here we present detailed observations of the gas and dust continuum of NGC1266 at millimeter wavelengths. Our observations show that molecular gas is being driven out of the nuclear region at


Astronomy and Astrophysics | 2010

A large 12C/13C isotopic ratio in M 82 and NGC 253

Sergio Martin; Rebeca Aladro; J. Martin-Pintado; R. Mauersberger

\dot{M}_{\rm out} \approx 110 M_\odot


The Astrophysical Journal | 2016

Discovery of a galaxy cluster with a violently starbursting core at z=2.506

Tao Wang; D. Elbaz; Emanuele Daddi; Alexis Finoguenov; Daizhong Liu; C. Schreiber; Sergio Martin; V. Strazzullo; Francesco Valentino; Remco F. J. van der Burg; Anita Zanella; Laure Ciesla; R. Gobat; Amandine M. C. Le Brun; M. Pannella; M. Sargent; Xinwen Shu; Qinghua Tan; N. Cappelluti; Yanxia Li

yr


Publications of the Astronomical Society of Japan | 2013

Submillimeter ALMA Observations of the Dense Gas in the Low-Luminosity Type-1 Active Nucleus of NGC1097

Takuma Izumi; Kotaro Kohno; Sergio Martin; Daniel Espada; Nanase Harada; Satoki Matsushita; Pei-Ying Hsieh; Jean L. Turner; David S. Meier; E. Schinnerer; Masatoshi Imanishi; Yoichi Tamura; Max T. Curran; Akihiro Doi; Kambiz Fathi; M. Krips; Andreas A. Lundgren; Naomasa Nakai; Taku Nakajima; Michael W. Regan; Kartik Sheth; Shuro Takano; Akio Taniguchi; Yuichi Terashima; Tomoka Tosaki; Tommy Wiklind

^{-1}


Astronomy and Astrophysics | 2015

Multimolecule ALMA observations toward the Seyfert 1 galaxy NGC 1097

Sergio Martin; Kotaro Kohno; Takuma Izumi; M. Kripsi; David S. Meier; R. Aladro; Satoki Matsushita; Shuro Takano; Jean L. Turner; Daniel Espada; Taku Nakajima; Yuichi Terashima; Kambiz Fathi; Pei-Ying Hsieh; Masatoshi Imanishi; A. Lundgren; Naomasa Nakai; E. Schinnerer; Kartik Sheth; Tommy Wiklind

, of which the vast majority cannot escape the nucleus. Only 2


The Astrophysical Journal | 2005

A New Intermediate-Mass Protostar in the Cepheus A HW2 Region

J. Martin-Pintado; Izaskun Jimenez-Serra; A. Rodriguez-Franco; Sergio Martin; Clemens Thum

M_\odot


The Astrophysical Journal | 2013

ALMA Follows Streaming of Dense Gas Down to 40?pc from the Supermassive Black Hole in NGC?1097

Kambiz Fathi; Andreas A. Lundgren; Kotaro Kohno; Nuria Pinol-Ferrer; Sergio Martin; Daniel Espada; Evanthia Hatziminaoglou; Masatoshi Imanishi; Takuma Izumi; M. Krips; Satoki Matsushita; David S. Meier; Naomasa Nakai; Kartik Sheth; Jean L. Turner; Glenn van de Ven; Tommy Wiklind

yr


Diabetes Research and Clinical Practice | 2008

Self-monitoring of blood glucose in type 2 diabetes: An inter-country comparison

S. Bot; Timothy M. E. Davis; Wendy A. Davis; A. Farmer; J.J. Gagliardino; C. Giorda; P.D. Home; G. Jermendy; L. Ji; John B. Johnson; A.J. Karter; H. Kolb; Sergio Martin; V. Mohan; A. Nicolucci; M. Porta; K.L. Ramaiya; J.H. Shah; A.S. Shera; S. Skeie

^{-1}


The Astrophysical Journal | 2016

SUBMILLIMETER-HCN DIAGRAM FOR ENERGY DIAGNOSTICS IN THE CENTERS OF GALAXIES

Takuma Izumi; Kotaro Kohno; Susanne Aalto; Daniel Espada; Kambiz Fathi; Nanase Harada; Bunyo Hatsukade; Pei-Ying Hsieh; Masatoshi Imanishi; M. Krips; Sergio Martin; Satoki Matsushita; David S. Meier; Naomasa Nakai; Kouichiro Nakanishi; E. Schinnerer; Kartik Sheth; Yuichi Terashima; Jean L. Turner

is actually capable of escaping the galaxy. Most of the molecular gas that remains is very inefficient at forming stars. The far-infrared emission is dominated by an ultra-compact (


The Astrophysical Journal | 2015

SIGNATURES OF YOUNG STAR FORMATION ACTIVITY WITHIN TWO PARSECS OF Sgr A

Farhad Yusef-Zadeh; Mark Wardle; Marta Malgorzata Sewilo; D. A. Roberts; I. Smith; Richard G. Arendt; W. D. Cotton; J. H. Lacy; Sergio Martin; Marc W. Pound; Matthew Rickert; M. Royster

\lesssim50

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Satoki Matsushita

Academia Sinica Institute of Astronomy and Astrophysics

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Susanne Aalto

Chalmers University of Technology

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J. Martin-Pintado

Spanish National Research Council

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David S. Meier

New Mexico Institute of Mining and Technology

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Daniel Espada

Graduate University for Advanced Studies

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Kazushi Sakamoto

Academia Sinica Institute of Astronomy and Astrophysics

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