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researcher

M. Ortega

44 papers hereh-index 11442 citations68 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author7
  • middle author22
  • last author10

Across the 39 of 44 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA41
  • astro-ph.HE2
  • astro-ph1
same name
  • M. Ortega — 16 papers, h 12
  • M. Ortega — 6 papers, h 25
  • M. Ortega — 5 papers, h 29
  • M. Ortega — 3 papers, h 0
  • M. Ortega — 1 paper, h 8
  • M. Ortega — 1 paper, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20082026
most citedA joint spectro-imaging analysis of the XMM-Newton and HESS observations of the supernova remnant RX J1713.7-3946

74 citations · 450 across the 44 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.GA2015★ 21 cited

A view of Large Magellanic Cloud HII regions N159, N132, and N166 through the 345 GHz window

S. Paron, M. E. Ortega, C. Fariña +3

We present results obtained towards the HII regions N159, N166, and N132 from the emission of several molecular lines in the 345 GHz window. Using ASTE we mapped a 2.4' × 2.…

astro-ph.GA2015★ 3 cited

The southern molecular environment of SNR G18.8+0.3

S. Paron, M. Celis Peña, M. E. Ortega +4

In a previous paper we have investigated the molecular environment towards the eastern border of the SNR G18.8+0.3. Continuing with the study of the surroundings of this SNR, in th…

astro-ph.GA2015★ 4 cited

HII region G46.5-0.2: the interplay between ionizing radiation, molecular gas and star formation

S. Paron, M. E. Ortega, G. Dubner +8

HII regions are particularly interesting because they can generate dense layers of gas and dust, elongated columns or pillars of gas pointing towards the ionizing sources, and come…

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