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Related papers: First Detection of HCO+ Emission at High Redshift

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We have mapped HCN and HCO$^{+}$ (J = 1 $\to$ 0) line emission toward a sample of seven star-forming regions (with 12 + log[O/H] range from 8.34 to 8.69) in the outer Milky Way (Galactocentric distance > 9.5 kpc), using the 14-meter radio…

Astrophysics of Galaxies · Physics 2022-09-14 Sudeshna Patra , Neal J. Evans , Kee-Tae Kim , Mark Heyer , Jens Kauffmann , Jessy Jose , Manash R. Samal , Swagat R. Das

We report new near-infrared and mm-wave observational data on a selection of massive Galactic molecular clumps (part of the CHaMP sample) and their associated young star clusters. The clumps show, for the first time in a "dense gas tracer",…

We present ALMA and VLA detections of the dense molecular gas tracers HCN, HCO$^+$ and HNC in two lensed, high-redshift starbursts selected from the {\it Herschel}-ATLAS survey: {\it H}-ATLAS\,J090740.0$-$004200 (SDP.9, $z \sim 1.6$) and…

We present new elements in the identification of the lens-system producing the 4 images of the BAL quasar H1413+117, based on the recent HST/NICMOS-2/F160W observations. After a careful PSF subtraction of the 4 images of the quasar, the…

Astrophysics · Physics 2007-05-23 J. -P. Kneib , D. Alloin , R. Pello

In recent years large efforts have been made to detect molecular gas towards high redshifted objects. Up to now the literature reports on only two cases of CO-detection in quasars at a redshift between 1 and 2 - Q0957+561, a gravitationally…

Astrophysics · Physics 2017-01-18 M. Krips , R. Neri , A. Eckart , J. Martin-Pintado , P. Planesas , L. Colina

We observed $\lambda$3mm \cotw, \coth, \coei, \hcop, HCN and CS emission from diffuse molecular gas along sightlines with \EBV\ $\approx$ 0.1 - 1 mag. Directions were mostly chosen for their proximity to sightlines toward background mm-wave…

Astrophysics of Galaxies · Physics 2020-07-15 Harvey S Liszt

We report results of a project to map HCN and HCO+ J = 1-0 emission toward a sample of molecular clouds in the inner Galaxy, all containing dense clumps that are actively engaged in star formation. We compare these two molecular line…

Astrophysics of Galaxies · Physics 2020-05-20 Neal J. Evans , Kee-Tae Kim , Jingwen Wu , Zhang Chao , Mark Heyer , Tie Liu , Quang Nguyen-Luong , Jens Kauffmann

We present here the sensitive HCN(1-0) observations made with the VLA of two submillimeter galaxies and two QSOs at high-redshift. HCN emission is the signature of dense molecular gas found in GMC cores, the actual sites of massive star…

Astrophysics · Physics 2009-11-13 Yu Gao , Chris L. Carilli , Philip M. Solomon , Paul A. Vanden Bout

We present 3 mm observations obtained with the IRAM 30-m telescope for ten nearby gas-rich active galaxies spanning three orders of magnitude in infrared luminosity. Emission lines of HCO+(1-0), HCN(1-0), and C2H(1-0) were simultaneously…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Xuejian Jiang , Junzhi Wang , Qiusheng Gu

We present a search for 183 GHz H_2O(3_13-2_20) emission in the infrared-luminous quasar MG 0751+2716 with the NRAO Very Large Array (VLA). At z=3.200+/-0.001, this water emission feature is redshifted to 43.6 GHz. As opposed to the faint…

The millimeter-wave rotational emission lines (4(04)-3(03) and 5(05)-4(04)) of protonated carbon dioxide, HCO2+(HOCO+), has been detected toward the low-mass class 0 protostar IRAS 04368+2557 in L1527 with the IRAM 30 m telescope. This is…

Astrophysics · Physics 2011-02-11 Nami Sakai , Takeshi Sakai , Yuri Aikawa , Satoshi Yamamoto

We present the first broadband lambda = 1 mm spectrum toward the z=2.56 Cloverleaf Quasar, obtained with Z-Spec, a 1-mm grating spectrograph on the 10.4-meter Caltech Submillimeter Observatory. The 190-305 GHz observation band corresponds…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 C. M. Bradford , J. E. Aguirre , R. Aikin , J. J. Bock , L. Earle , J. Glenn , H. Inami , P. R. Maloney , H. Matsuhara , B. J. Naylor , H. T. Nguyen , J. Zmuidzinas

We present the detection of carbon monoxide molecules (CO) at z=1.6408 towards the quasar SDSSJ160457.50+220300.5 using the VLT Ultraviolet and Visual Echelle Spectrograph. CO absorption is detected in at least two components in the first…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 P. Noterdaeme , C. Ledoux , R. Srianand , P. Petitjean , S. Lopez

We present 3 mm and 2 mm band simultaneously spectroscopic observations of HCN 1-0, HCO$^{+}$ 1-0, HNC 1-0, and CS 3-2 with the IRAM 30 meter telescope, toward a sample of 70 sources as nearby galaxies with infrared luminosities ranging…

Astrophysics of Galaxies · Physics 2021-03-24 Fei Li , Junzhi Wang , Feng Gao , Shu Liu , Zhi-Yu Zhang , Shanghuo Li , Yan Gong , Juan Li , Yong Shi

We report the detection of luminous CO(2-1), CO(3-2), and CO(4-3) emission in the strongly lensed high-redshift quasars B1938+666 (z=2.059), HE0230-2130 (z=2.166), HE1104-1805 (z=2.322), and B1359+154 (z=3.240), using the Combined Array for…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-18 Dominik A. Riechers

We report observations of dense molecular gas in the star-forming galaxy EGS 13004291 (z=1.197) using the Plateau de Bure Interferometer. We tentatively detect HCN and HNC (J=2-1) emission when stacked together at ~4sigma significance,…

Astrophysics of Galaxies · Physics 2017-04-12 Avani Gowardhan , Dominik A. Riechers , Emanuele Daddi , Riccardo Pavesi , Helmut Dannerbauer , Chris Carilli

We report our new observations of redshifted carbon monoxide emission from six z~6 quasars, using the PdBI. CO (6-5) or (5-4) line emission was detected in all six sources. Together with two other previous CO detections, these observations…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Ran Wang , Chris L. Carilli , R. Neri , D. A. Riechers , Jeff Wagg , Fabian Walter , Frank Bertoldi , Karl M. Menten , Alain Omont , Pierre Cox , Xiaohui Fan

We detect luminous emission from HCN, HCO+ and HNC 1--0 in the QSO ULIRG Mrk~231 with the IRAM Plateau de Bure Interferometer at 1."55 by 1."28 resolution. All three lines show broad line wings - which are particularly prominent for HCN.…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 S. Aalto , S. Garcia-Burillo , S. Muller , J. M. Winters , P. van der Werf , C. Henkel , F. Costagliola , R. Neri

It has been recently argued that the HCN J=1--0 line emission may not be an unbiased tracer of dense molecular gas ($\rm n\ga 10^4 cm^{-3}$) in Luminous Infrared Galaxies (LIRGs: $\rm L_{FIR}> 10^{11} L_{\odot}$) and HCO$^+$ J=1--0 may…

Astrophysics · Physics 2008-11-26 Padelis P. Papadopoulos

Both Galactic and extragalactic studies on star formation suggest that stars form directly from dense molecular gas. To trace such high volume density gas, HCN and HCO+ J=1-0 have been widely used for their high dipole moments, relatively…

Astrophysics of Galaxies · Physics 2022-09-07 Jing Zhou , Zhi-Yu Zhang , Yu Gao , Junzhi Wang , Yong Shi , Qiusheng Gu , Chentao Yang , Tao Wang , Qinghua Tan